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1 act as nucleation sites for further growth by molecular accretion.
2 artitioning of lead into the core throughout the Earth's accretion.
3 llar core and find that radiation pressure does not halt accretion.
4 t has long been expected to prevent them from growing by accretion.
5 5(OH)D and calcium levels but does not improve bone mass accretion.
6 ffspring growth, which is suggestive of lean tissue mass accretion.
7 nvolved in capsomere-capsomere interactions during shell accretion.
8 pectral curvature are indeed signatures of supercritical accretion.
9 sk to shed angular momentum that would otherwise inhibit accretion.
10 standing of how to limit proteolysis and promote protein accretion.
11 the theoretic energy required for age-appropriate tissue accretion.
12 nd 4E-BP1 (gel shift), as well as deficits in total eEF2 accretion.
13 of mass subsequently added during the era known as Late Accretion.
14 r system and transported to the Kuiper belt before comet accretion.
15 which we conclude that high-mass stars can form through accretion.
16 itationally pull in surrounding gas, in a process called accretion.
17 ernal cholesterol can affect fetal metabolism and sterol accretion.
18 seems to be due to the sudden onset of a phase of rapid accretion.
19 e mass of chondritic material added to Earth during Late Accretion.
20 solated at the core-mantle boundary region since Earth's accretion.
21 budgets typically become net negative and threaten reef accretion.
22 ltering concentrations of hormones that regulate mineral accretion.
23 ets are expected to have higher spin rates at the end of accretion.
24 al fat, prevented bone loss, and improved lean body mass accretion.
25 l, hepatic, and splenic uptake while not affecting tumor accretion.
26 low fO(2) during Earth (and other differentiated bodies) accretion.
27 studies of black holes have revealed a complex array of accretion activity, the mechanisms that trigger and suppre
28 ssess the effects on calcium absorption and bone mineral accretion after 8 wk and 1 y of supplementation with an in
29 If there is accretion after neutron-star formation, the atmosphere cou
30 obtained from Hf-W systematics, and implies substantial accretion after the Moon-forming impact, which occurred 45
31 the long-term effects of calcium supplementation on bone accretion among females from childhood to young adulthood.
32 This may lead to a lack of normal bone mineral accretion and a subsequent reduction in the lumbar spine B
33 ing flux and the basal mass balance (the balance between accretion and ablation at the ice-shelf base) for the whol
34 The phenomenon is known as pulsed accretion and can affect the orbital evolution and mass di
35 We have developed a 3D model of tidal marsh accretion and channel network development that couples phy
36 Measurements of its size distribution constrain its accretion and collisional history, and the importance of m
37 tion during accretion, and related to current models for accretion and core formation in the Earth.
38 he processes that occurred during the last 1% of Earth's accretion and core formation in the Wood and Halliday mech
39 clocks (30 Myr) in determining the timescale of Earth's accretion and core formation.
40 The rate of accretion and core segregation on Earth as deduced from th
41 or constraining the fundamental processes of protoplanet accretion and differentiation within the solar protoplanet
42 by ordered beta-sheet linkages leading to intracellular accretion and disease.
43 d intrachain hydrogen bonding guides secondary structure accretion and DSE contraction as solvent quality is decrea
44 e indeed at an early evolutionary stage, with rapid mass accretion and dust formation.
45 ection has erased the signature of Earth's heterogeneous accretion and early differentiation.
46 ry mechanism of segment growth and that focused magmatic accretion and extension in the crust have remained stable
47 galaxies and their nuclear massive black holes, through accretion and galactic merging.
48 light the need for caution when modelling reef framework accretion and interpreting results which extrapolate infor
49 e Earth had a protracted and complex history of volatile accretion and loss.
50 We focus on the clear empirical rules connecting accretion and outflow that have been established for stell
51 thought to have been fixed by a complex interplay of gas accretion and protostellar radiation.
52 lutionary scenario for the DdRp subunits includes domain accretion and rearrangement, with some likely horizontal t
53 is dictated by the competition between vertical sediment accretion and relative sea-level rise.
54 and dark matter sink to the centres of galaxies through accretion and repeated mergers.
55 This structure is important for shell accretion and stability of the protein coat.
56 double-stranded DNA phages, are a key regulator of shell accretion and stabilization.
57 Muscle protein accretion and synthesis were measured with the femoral art
58 ontrolling the acquisition of volatiles during planetary accretion and their subsequent evolution.
59 hypothesis assumes non-linear relationships between peat accretion and water depth, and describes flow-dependent fe
60 ism because high-calcium diets attenuate adipocyte lipid accretion and weight gain during the overconsumption of an
61 that the U-Pb age cannot be used to argue for protracted accretion and/or core formation (>50 Myr) because this clo
62 ns-domain containing protein: GLR-1 accumulates in large accretions and animals display a decreased frequency of re
63 e effect of enteral nutrition on proteolysis and protein accretion, and conducting a large randomized controlled tr
64 ion-year history, such as formation of the first solids, accretion, and differentiation of protoplanetary bodies, h
65 gene duplication and triplication, exon shuffling, exon accretion, and fusion/fission events.
66 increasing P and T, changing silicate composition during accretion, and related to current models for accretion and
67 star-forming region can undergo significant competitive accretion, and that the simulations that show competitive
68 Mid-ocean ridge morphology and crustal accretion are known to depend on the spreading rate of the
69 or materials, extent of mixing, and material loss during accretion are poorly constrained.
70 riven by intense bursts of star formation and black hole accretion, are processes invoked by current theories of ga
71 Here we derive the rate of competitive accretion as a function of the star-forming environment, b
72 d with core formation, or from evaporative losses during accretion as the planets were built up.
73 We attribute this to pulsed accretion associated with an unseen binary companion.
74 proximately 30 Myr, corresponds to the end of main-stage accretion at approximately 30 Myr.
75 tents among these bodies, therefore, did not result from accretion at different times from an incompletely condense
76 We propose that ZO-1 controls the rate of Cx43 channel accretion at GJ peripheries, which, in conjunction with th
77 high-mineral-containing formulas allows for bone mineral accretion at or near in utero rates.
78 offer the best constraints on early stages of planetary accretion because most are remnants of the oldest bodies,
79 st existed as early as 150 million years after planetary accretion, but assessing the rates and processes of subseq
80 Mass accretion by black holes (BHs) is typically capped at the
81 torage proteins found in maize (Zea mays), accumulate in accretions called protein bodies inside the endoplasmic re
82 nto the timing and nature of collisions during planetary accretion can be gained from meteorite studies.
83 and determine in what types of environments competitive accretion can occur.
84 eature is interpreted to be the result of a post-primary-accretion cataclysmic spike in the number of impacts commo
85 arguing that the source is highly compact and powered by accretion close to the Eddington limit onto a black hole o
86 otomy formation time approximately 100 Myr after martian accretion, comparable to that of the Moon-forming impact o
87 Juvenile recruitment and reef accretion correlated with oyster density, facilitating ree
88 X-ray spectral regions from stellar debris that forms an accretion disk around the black hole.
89 Subsequent formation of a super-Eddington accretion disk from the disrupted companion inside a commo
90 etion disk, suggesting that the M87 jet is powered by an accretion disk in a prograde orbit around a spinning black
91 on line in the quasar PG 1700+518 originate close to the accretion disk in an electron scattering wind.
92 Here we report that jet magnetic field and accretion disk luminosity are tightly correlated over seve
93 instability is believed to episodically dump much of the accretion disk onto the white dwarf.
94 lds twisted by differential rotation of the black hole's accretion disk or inertial-frame-dragging ergosphere.
95 ds probably play a critical role in jet formation and in accretion disk physics.
96 ries of magnetic collimation, the predicted structure on accretion disk scales at the jet launch point has not been
97 Winds launched from a rotating accretion disk surrounding the black hole are thought to p
98 Such baryonic jets are more likely to be powered by the accretion disk than by the spin of the black hole, and if
99 These fields obstruct gas infall, compress the accretion disk vertically, slow down the disk rotation by
100 The circumstellar accretion disk was evaporated by ultraviolet radiation fro
101 erextended infrared star or, later, a black hole with an accretion disk, although the preferred interpretation was
102 ficantly smaller than the innermost edge of a retrograde accretion disk, suggesting that the M87 jet is powered by
103 r the removal of high-angular-momentum material from the accretion disk, thereby allowing the central protostar to
104 a red dwarf transfers hydrogen-rich matter, by way of an accretion disk, to its white dwarf companion.
105 ndom motions suppress the formation of a slowly draining accretion disk.
106 on field around the black hole drives a hot wind off the accretion disk.
107 emission line arises when the jet illuminates the inner accretion disk.
108 field lines and centrifugally accelerated off a rotating accretion disk.
109 study of relativistic reflection features from the inner accretion disk.
110 days from the nucleus, it may likely originate from the accretion disk.
111 approximately 5-20M cicled dot, probably by means of an accretion disk.
112 It is unclear, however, whether the accretion-disk paradigm can also account for the formation
113 deal nearby 'laboratories' for studying the evolution of accretion disks and jet formation in black-hole systems.
114 Accretion disks must transfer angular momentum in order fo
115 Magnetic fields in accretion disks play a dominant part during the star forma
116 Tauri stars and possibly in the innermost part of their accretion disks, but the strength and morphology of the fi
117 al mass ejections) and predicted (the inner heliosheath, accretion disks, gamma-ray bursts and so on).
118 Scaled to accretion disks, rates of angular momentum transport lie f
119 most efficient energy sources known in the Universe are accretion disks.
120 ccretion, and that the simulations that show competitive accretion do so because the assumed properties differ from
121 saccharide (K1 antigen), which is encoded by the kps/neu accretion domain inserted near pheV at 67 map units.
122 rt-term studies established that calcium influences bone accretion during growth.
123 ietary calcium requirements for maximal skeletal calcium accretion during puberty may differ between the races.
124 Here we show that NO accretion during the nitrosative burst promotes increasing
125 In utero rates of calcium accretion during the third trimester cannot be readily ach
126 Thus, discharge competence and non-linear peat accretion dynamics may explain the establishment, persiste
127 Late accretion, early mantle differentiation, and core-mantle i
128 he endo-neuraminidase tail protein gene of a chromosomal accretion element, designated CUS-3, with homology to lamb
129 We suggest that such accretion-enhanced X-ray emission from erupting young star
130 </= 1 occurs principally by coherent rather than chaotic accretion episodes.
131 racteristics, we show that observations suggest a sudden accretion event onto a central MBH of mass about 10(6) to
132 n added early to Earth, rather than gained during a late accretion event.
133 49.3+573451) was found, potentially representing such an accretion event.
134 Observational evidence of accretion events is provided by the coherent stellar strea
135 Previous hypotheses for its origin have included late accretion events, large impacts, tidal effects and convect
136 Wind accretion explains the X-ray luminosity, and the black-hol
137 dly relativistic ejecta, along with a central engine (an accretion-fed, rapidly rotating compact source) that produ
138 ources should reveal the causal relationship between the accretion flow and the powerful jet emission.
139 ine further suggests the presence of an outflow from the accretion flow onto the SMBH.
140 ronomical goal is to resolve structures in the innermost accretion flow surrounding Sgr A*, where strong gravitatio
141 centred on the black hole, but arises in the surrounding accretion flow.
142 the characteristic rapid X-ray variability seen from the accretion flow.
143 rgy strongly influences the geometry and dynamics of the accretion flow.
144 high spin found here is indicative of growth by coherent accretion for this black hole, and suggests that black-hol
145 a ring originating in the break-up of a larger body, but accretion from a circumplanetary disk is also plausible if
146 ypothesis but is well explained by the standard model of accretion from partially volatile-depleted material, accom
147 Periodic variations consistent with pulsed accretion have been seen in only a few young binaries via
148 on takes place or if thermonuclear reactions occur after accretion, heavy elements (for example, Fe) are expected.
149 of the SMBHs, which often comes in the form of long-term accretion in active galactic nuclei.
150 diabetes, hepatic steatosis, hyperlipidemia, and adipose accretion in animal models of obesity.
151 owed intense uptake within the tumors and no evidence of accretion in any normal tissue.
152 girls, yet it is unknown whether the additional skeletal accretion in boys requires additional dietary calcium inta
153 nutrition in limiting proteolysis and producing protein accretion in preterm infants, but the protein content of c
154 hat intense asteroidal deformation accompanied planetary accretion in the early Solar System.
155 a dynamical mechanism that can trigger supra-exponential accretion in the early universe, when a BH seed is bound i
156 Abnormal fat accretion in the setting of obesity can lead to insulin re
157 Whether long-term supplementation influences bone accretion in young adults is not known.
158 supplemental dietary fatty acid that decreases fat mass accretion in young animals.
159 Calcium supplementation significantly influenced bone accretion in young females during the pubertal growth spur
160 o to three generations, accompanied by filamentation and accretion (in approximately 2% of cells) of paracrystallin
161 Liver fat accretion, independent of VAT, may play a role in the ethn
162 ent, which shows the effectiveness of ALA conversion and accretion into erythrocytes.
163 s peak epoch of cosmic star formation indicates that gas accretion is likely to be the dominant mode by which galax
164 activity with age), to X-ray generating processes (e.g., accretion, jets, magnetically confined winds) that were po
165 black holes are thought to grow mostly by merger-driven accretion leading to high spin.
166 sustaining the inner disk (around GG Tau Aa) beyond the accretion lifetime, leaving time for planet formation to o
167 ia optical accretion tracers, albeit intermittently with accretion luminosity variations ranging from zero to 50 pe
168 is finding in turn suggests that three-dimensional magma accretion may occur near intermediate- and fast-slipping t
169 Late accretion may offer a solution, provided that >/=0.5% Eart
170 rain differences in adipokines and myocardial fatty acid accretion may underlie heterogeneous data from rodent stud
171 challenge of detecting the donor against the light from accretion, means that no donor star to date has a measured
172 The survey measurements support the core accretion model, in which planets form by the accumulation
173 ns have failed to confirm predictions of the competitive accretion model.
174 agnetars to ordinary radio pulsars, rule out alternative accretion models for AXPs, and provide a new window into t
175 Competitive accretion models interpret brown dwarfs and free-floating
176 eroid belt, ancient martian impact basins, and planetary accretion models.
177 us-like nephritis (n = 2), and urinary calcium carbonate accretions (n = 3) were seen in animals with high exposure
178 this finding suggests that two distinct modes of crustal accretion occur along slow-spreading ridges.
179 Mars' accretion occurred early enough to allow establishment of
180 tcatalytic transit through the protein cage, and mineral accretion occurs in the central cavity.
181 e we consider its origin as a late carapace added by the accretion of a companion moon.
182 The flare of radiation from the tidal disruption and accretion of a star can be used as a marker for supermassi
183 logy suggests that the role of the magnetic field in the accretion of a T Tauri star is more complex than our curre
184 This possibly involves accretion of additional Tha4 into a larger transport-activ
185 The accretion of bodies in the asteroid belt was halted nearly
186 crucial role in the assimilation of dietary fat and the accretion of body fat in mice.
187 processes of planetary formation by mediating the rapid accretion of disk material onto the central star and the f
188 Accretion of domains and molecules gave rise to modern aaR
189 182)Hf-(182)W chronometry of terrestrial rocks points to accretion of Earth in approximately 30 Myr after the forma
190 s holds particular promise for clarifying the sequential accretion of ecological and behavioral characters that pro
191 es of orogenesis and crustal shortening, coincident with accretion of exotic crust.
192 at postnatal stages when fibrils increase in diameter by accretion of extracellular collagen, thereby maintaining p
193 low-energy efficiency of protein); and 3) maintenance or accretion of fat-free mass--in some individuals, a moderat
194 f a parent asteroid, with the new primary resulting from accretion of fragments, while the moonlets are formed from
195 (40) erg s(-1); ref. 1) are thought to be powered by the accretion of gas onto black holes with masses of approxima
196 ates vast radiant luminosities through the gravitational accretion of gas.
197 indicates that CpG and NFI sites emerged with a general accretion of GC-rich sequences downstream of the eukaryoti
198 results support horizontal transfer as the mechanism for accretion of genes into the PAI and highlight a likely rol
199 This suggests that the C-terminal domain mediates an accretion of HMO1 on DNA that causes in-phase DNA bending
200 embly models: one allowing growth to proceed only by the accretion of individual assembly subunits and the other al
201 ircumgalactic medium (CGM) is fed by galaxy outflows and accretion of intergalactic gas, but its mass, heavy elemen
202 atic front, supports cratonic assembly by subduction and accretion of lithospheric fragments.
203 nt studies suggest that high-mass stars may form through accretion of material from a circumstellar disk, in essent
204 The accretion of matter onto a massive black hole is believed
205 ay population, and it challenges physical models for the accretion of matter onto magnetized compact objects.
206 clei exhibit relativistic jets, which are powered by the accretion of matter onto supermassive black holes.
207 e C-terminal domain mediates both DNA end-joining and an accretion of multiple HMO1 protomers on duplex DNA that pr
208 These data indicate that aging results in a diminished accretion of muscle proteins after ingestion of a small do
209 of a smaller bolus of EAAs is associated with diminished accretion of muscle proteins in the elderly when compared
210 ng the individual mutations, showing that the systematic accretion of mutations can yield progressive increases in
211 e used to identify genes differentially regulated during accretion of P. gingivalis in heterotypic biofilms with S.
212 specific protein-protein interactions contribute to the accretion of plasma proteins during drusen formation.
213 Late accretion of primitive chondritic material to Earth, the M
214 Diminished accretion of SHF precursors to the elongating OFT myocardi
215 structural rearrangement and three-dimensional growth by accretion of silica molecules.
216 alysis of all well populated CATH families, suggest that accretion of small secondary structure insertions may prov
217 ed to grow continuously through hierarchical merging and accretion of smaller systems.
218 by ~7%, probably via non-mass-dependent chemistry before accretion of the first planetesimals.
219 d-crustal lenses at the spreading axis, but the style of accretion of the lower oceanic crust is actively debated.
220 We assumed that accretion of the outer portion of the stellar core by a ce
221 ized on Earth, at least since the termination of primary accretion of the planets and the postulated impact origin
222 ck hole fuels the prompt emission and that fall-back and accretion of the stellar envelope later produce the platea
223 frican-Americans appear to be more resistant to both the accretion of triglyceride in the abdominal visceral compar
224 at final stellar masses are determined by the subsequent accretion of unbound gas from the clump.
225 The abundant accretion of vascular amyloid, despite low AbetaPP transge
226 nitrification appears to constrain the extent of nitrate accretion, once organic carbon and nitrate availability ap
227 newly formed relativistic outflow, launched by transient accretion onto a million-solar-mass black hole.
228 Transient accretion onto a supermassive black hole, for example thro
229 This result demonstrates that disk accretion onto black holes is a fundamentally magnetic pro
230 tive galactic nuclei (AGN) shone brightly as a result of accretion onto black holes.
231 Active galactic nuclei, which are powered by long-term accretion onto central supermassive black holes, produce r
232 Although disk accretion onto compact objects-white dwarfs, neutron stars
233 10(40) ergs per second can be explained by supercritical accretion onto massive stellar-mass black holes.
234 Gas accretion onto some massive black holes (MBHs) at the cent
235 -up versions of Galactic black hole binaries, powered by accretion onto supermassive black holes with masses of 10(
236 errestrial planet formation, giant planet migration, and accretion onto the central star.
237 ested that X-ray emission may be a direct result of mass accretion onto the forming star.
238 dence for a causal link between gas-rich galaxy mergers, accretion onto the nuclear SMBH, and coeval star formation
239 Given that the inner disks are depleted by accretion onto the stars on timescales of a few thousand y
240 south, suggesting that erosion, not subcrustal sediment accretion or anatexis, is partly responsible for the thick
241 imately 1 these black holes continue to grow by coherent accretion or in a chaotic manner, though clear differences
242 ion of the basal thermal regime of the ice sheet by lake accretion or through scouring bedrock channels in periodic
243 ithic collisional shards, modified to varying degrees by accretion, or may have grown by accretion without the aid
244 ute periodontitis, chronic periodontitis, periodontosis, accretions, other specified periodontal disease, or unspec
245 hich indicated greater fat mass accretion than lean mass accretion (P < 0.001).
246 sembly mechanisms, a standard nucleation-limited monomer-accretion pathway and two distinct hierarchical assembly p
247 ent growth onto large particles occurs after the primary accretion phase has concluded.
248 onto and away from protostars during their initial mass accretion phase.
249 timescales can be physically linked, revealing that the accretion process is exactly the same for small and large
250 ude that most of the luminosity is generated through the accretion process, with an accretion rate of about 6.6 x 1
251 tio'), which is an important parameter of the black hole accretion process.
252 nearly circular orbits, as is expected if they formed by accretion processes in a protostellar disk.
253 Although generally associated with the accretion processes necessary for marshes to keep up with
254 This implies that stars of all masses can form via accretion processes, and coalescence of intermediate-mass
255 The high gas opacity traps the accretion radiation, while the low-mass BH's random motion
256 e and decay of the light curve follow the predicted mass accretion rate and can be modelled to determine the time o
257 sity is generated through the accretion process, with an accretion rate of about 6.6 x 10(-7) solar masses per year
258 The terrestrial IDP accretion rate was overwhelmingly dominated by Veritas fam
259 e we report that, after correcting for variations in the accretion rate, the timescales can be physically linked, r
260 Calculated accretion rates (mm year(-1)) for shallow fore-reef habita
261 oximately 300,000 years, although theory suggests larger accretion rates earlier, so it may be younger.
262 e model builds a marsh platform and channel network with accretion rates everywhere equal to the rate of sea-level
263 Periodic increases in luminosity arising from variable accretion rates have been predicted for some pre-main-sequ
264 f(intact))) were similar and concordant with net calcium accretion rates in vivo.
265 , exactly as expected from the AGN black hole masses and accretion rates.
266 sion from young stars can occur as a consequence of high accretion rates.
267 alaxies such as the Milky Way gain much of their mass by accretion rather than major mergers.
268 system, not only the asteroid belt but even in the comet accretion region, suggesting a huge and efficient process
269 Here we report a robust instability of the stalled accretion shock in core-collapse supernovae that is able t
270 The strength and regularity of this accretion signal is surprising; it may be related to the v
271 is inversely correlated with the time scale of the main accretion stage of the Earth.
272 ints for models of the prevalent radiatively inefficient accretion state.
273 Accretion stops, and the pre-main sequence star that emerg
274 a contains a reef-like assembly of laminated sedimentary accretion structures (stromatolites) that have macroscale
275 ere could be composed of light elements (H or He); if no accretion takes place or if thermonuclear reactions occur
276 ass ratio was observed, which indicated greater fat mass accretion than lean mass accretion (P < 0.001).
277 ue or significant departures from the standard thin disk accretion that powers bright Galactic X-ray binaries, or b
278 ion in both bodies, followed by post-core-formation late accretion that replenished their mantles with highly sider
279 The lunar mantle experienced late accretion that was similar in composition to that of Earth
280 ed by radioactive decay and was only incorporated during accretion-that is, it is primordial.
281 This is in good agreement with the core-accretion theory of planet formation, in which a gas giant
282 In contrast, competitive accretion theory suggests that at birth all stars are much
283 ust be powered by a magnetic process that can also drive accretion through the disk.
284 Fast accretion times there allowed small planetesimals to melt
285 To assess this idea, it is crucial to know Mars' accretion timescale, which can be investigated using the (
286 nd that the polymer can increase the net rate of subunit accretion to a growing capsid both by stabilizing the addi
287 te MGI (> 52 Myr) requires the main stage of the Earth's accretion to be completed rapidly in < 10.7 +/- 2.5 Myr.
288 t limit stellar masses, but the instabilities that allow accretion to continue lead to small multiple systems.
289 However, at high redshifts we require active, continuous accretion to infer the presence of the SMBHs, which often
290 The timing of water accretion to the inner solar system also has implications
291 have been seen in only a few young binaries via optical accretion tracers, albeit intermittently with accretion lu
292 Accretion variability is a common feature of young stars,
293 Bone mineral accretion was lower (P = 0.04) in the CLA group (0.05 +/-
294 Calcium accretion was significantly elevated in NL fetuses by 19 d
295 1/Ser424), 4E-BP1 phosphorylation status, and total eEF2 accretion were all positively correlated with percentage m
296 d strontium isotope data are reconciled by heterogeneous accretion, which includes a transition from dominantly vol
297 signaling pathway, and fibrogenesis despite similar fat accretion with diet-induced obesity.
298 Determining the origin of water and the timing of its accretion within the inner solar system is important for u
299 n the hydrodynamic radius (R(h)) and secondary structure accretion without populating the native state.
300 ed to varying degrees by accretion, or may have grown by accretion without the aid of a core.

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