ライフサイエンスコーパス: accretion

1 stimulate insulin-mediated muscle carnitine accretion.

2 positive protein balance and skeletal muscle accretion.

3 pread land loss, and vertical marsh sediment accretion.

4 a necessary counterpart to protostellar mass accretion.

5 pth and processes occurring during planetary accretion.

6 imiting steps of hepatic glucose release and accretion.

7 sequently added during the era known as Late Accretion.

8 ding combined with local cell ingression and accretion.

9 ature are indeed signatures of supercritical accretion.

10 quently depleted in volatile elements during accretion.

11 orticosteroid treatment slightly reduced FFM accretion.

12 ondritic material added to Earth during Late Accretion.

13 is required to support healthy bone mineral accretion.

14 le-rich or water-rich late-stage terrestrial accretion.

15 ically become net negative and threaten reef accretion.

16 he core-mantle boundary region since Earth's accretion.

17 e to a selective reduction in adipose tissue accretion.

18 oor spreading compared to classical magmatic accretion.

19 entrations of hormones that regulate mineral accretion.

20 tic plasticity defects caused by tau's toxic accretion.

21 of these volatiles, or addition through late accretion.

22 p to slow hindlimb growth and muscle protein accretion.

23 cted to have higher spin rates at the end of accretion.

24 sphere during the last stages of terrestrial accretion.

25 ented bone loss, and improved lean body mass accretion.

26 and splenic uptake while not affecting tumor accretion.

27 (4) solar masses or episodic hyper-Eddington accretion.

28 , 20%, or 50%, in increasing fat-free tissue accretion.

29 its association with Std1 and triggers Std1 accretion.

30 e provided by ongoing mergers or cold-stream accretion.

31 e spatially variable patterns of erosion and accretion along the large deltas of the main rivers in t

32 the basal mass balance (the balance between accretion and ablation at the ice-shelf base) for the wh

33 thesis, suggesting a link between myonuclear accretion and activation of pro-hypertrophic pathways.

34 were E-type in the first 60 per cent of the accretion and all of the impactors were E-type after tha

35 e analog oxandrolone improves lean body mass accretion and bone mineral content and that the administ

36 The phenomenon is known as pulsed accretion and can affect the orbital evolution and mass

37 sitive over summer and negative over winter, accretion and catabolism of those reserves was not consi

38 Differential nanotube accretion and clearance from critical organs have been o

39 ing the fundamental processes of protoplanet accretion and differentiation within the solar protoplan

40 rased the signature of Earth's heterogeneous accretion and early differentiation.

41 of segment growth and that focused magmatic accretion and extension in the crust have remained stabl

42 statin, a known inhibitor of skeletal muscle accretion and growth.

43 ed for caution when modelling reef framework accretion and interpreting results which extrapolate inf

44 ocus on the clear empirical rules connecting accretion and outflow that have been established for ste

45 that amplifies weak magnetic fields, driving accretion and outflow.

46 n through regulation of centriolar satellite accretion and Rab8a.

47 by the competition between vertical sediment accretion and relative sea-level rise.

48 esent-day surface-elevation change, vertical accretion and shallow subsidence rates.

49 Critical measurements for understanding accretion and the dust/gas ratio in the solar nebula, wh

50 ys in which mangroves may influence sediment accretion and vertical land development, for example, th

51 ssumes non-linear relationships between peat accretion and water depth, and describes flow-dependent

52 In contrast to current notions of summer accretion and winter catabolism of body reserves, some i

53 y experience decreased soil OM accumulation, accretion, and carbon sequestration rates even with mode

54 ve biomarkers of metabolic health, limit fat accretion, and enhance insulin sensitivity.

55 fosl2 mutants initiate accretion appropriately, but cardiomyocyte production is

56 al ages played an equal role in absolute FFM accretion, as did the initial growth (between birth and

57 We attribute this to pulsed accretion associated with an unseen binary companion.

58 these bodies, therefore, did not result from accretion at different times from an incompletely conden

59 that genetic determinants of childhood bone accretion at the radius, a skeletal site that is primari

60 an a billionth of a solar mass per year, the accretion becomes unstable and the matter is dumped onto

61 es were detectable in adipose tissue or IHCL accretion between breastfed and formula-fed infants up t

62 ation protects mice specifically against fat accretion but not against other pathological side effect

63 ant contributor for deltaic wetland vertical accretion, but the contribution from hurricanes to long-

64 Mass accretion by black holes (BHs) is typically capped at th

65 of relative sea-level rise (RRSLR), surface accretion by inorganic sediment deposition, and organic

66 theory and simulations instead predict that accretion can be dominated by a stochastic, clumpy distr

67 Because of the importance of accretion chemistry, the aerosol yield from D5 oxidation

68 the source is highly compact and powered by accretion close to the Eddington limit onto a black hole

69 Using a Monte Carlo accretion code, we estimate the location, timing, sizes,

70 sufficiently large to direct the flow as an accretion column onto the poles of the white dwarf, a st

71 for carbonaceous chondrites reveal that late accretion, constrained to a maximum of 0.5 +/- 0.2 per c

72 stars, for which similar magnetically gated accretion cycles have been identified.

73 ep Earth have implications, not only for its accretion-differentiation history but also for carbon is

74 lo--electron volts), which is ascribed to an accretion disk corona of energetic particles akin to tho

75 e their ubiquity, the physical conditions in accretion disk coronae remain poorly constrained.

76 is responding to the emission from the inner accretion disk demonstrates a connection between accreti

77 winds of ionized material, expelled from the accretion disk encircling the black hole, and collimated

78 suggesting that the M87 jet is powered by an accretion disk in a prograde orbit around a spinning bla

79 hole, differential rotation of a magnetized accretion disk is thought to produce an instability that

80 Here we report that jet magnetic field and accretion disk luminosity are tightly correlated over se

81 play a critical role in jet formation and in accretion disk physics.

82 by the progenitors, whose pre-main-sequence accretion disk suffered an early disruption in the dense

83 ic jets are more likely to be powered by the accretion disk than by the spin of the black hole, and i

84 ese fields obstruct gas infall, compress the accretion disk vertically, slow down the disk rotation b

85 we report observations of a sustained outer accretion disk wind in V404 Cyg, which is unlike any see

86 pelled at relativistic speeds from the inner accretion disk, and its wide aperture suggests an effect

87 e inner, super-Eddington region of a nascent accretion disk, or with a filament of disrupted stellar

88 ller than the innermost edge of a retrograde accretion disk, suggesting that the M87 jet is powered b

89 he nucleus, it may likely originate from the accretion disk.

90 suppress the formation of a slowly draining accretion disk.

91 ativistic reflection features from the inner accretion disk.

92 ly 5-20M cicled dot, probably by means of an accretion disk.

93 ly 5-20M cicled dot, probably by means of an accretion disk.

94 sion of X-rays from the inner regions of the accretion disk.

95 ass flow into the inner regions of its large accretion disk.

96 s between large-scale molecular outflows and accretion-disk activity in ultraluminous galaxies were i

97 kes but much lower mass-transfer rates, when accretion-disk instabilities drop matter onto the white

98 luminous galaxies were incomplete because no accretion-disk wind had been detected.

99 Here we report observations of a powerful accretion-disk wind with a mildly relativistic velocity

100 Conversely, studies of powerful accretion-disk winds have until now focused only on X-ra

101 te as energy-conserving flows driven by fast accretion-disk winds.

102 haotically in the binary potential and forms accretion disks around both black holes.

103 retion phases shown by transients with large accretion disks imply that this outflow is probably a fu

104 Magnetic fields in accretion disks play a dominant part during the star for

105 and possibly in the innermost part of their accretion disks, but the strength and morphology of the

106 tions) and predicted (the inner heliosheath, accretion disks, gamma-ray bursts and so on).

107 that matter is absorbed into black holes via accretion disks, the state of which depends primarily on

108 s born preterm and suggests that ectopic fat accretion driven by their relatively greater adiposity m

109 tion in clusters, but it is not known how an accretion-driven jet or outflow in a clustered environme

110 The data suggest that episodic, accretion-driven outflow begins in the earliest phase of

111 d of light and triggers a nebular phase once accretion drops sharply and the ejecta become optically

112 e significantly associated with absolute FFM accretion during a hospital stay in preterm infants.

113 -type exercise stimulates net muscle protein accretion during acute postexercise recovery.

114 itudinal association between growth and bone accretion during childhood is not fully understood.

115 e one such dietary factor that promotes bone accretion during early life with persistent effects into

116 e expected to experience outbursts caused by accretion during their formation, our results imply that

117 us, discharge competence and non-linear peat accretion dynamics may explain the establishment, persis

118 ic field that is strong enough to affect the accretion dynamics.

119 principally by coherent rather than chaotic accretion episodes.

120 in coral-sponge interactions can alter reef accretion/erosion balance and are important to predict t

121 ls experienced similar primordial stratified accretion, even though they formed independently.

122 y to Earth, rather than gained during a late accretion event.

123 Observational evidence of accretion events is provided by the coherent stellar str

124 hypotheses for its origin have included late accretion events, large impacts, tidal effects and conve

125 gas accretes into those dwarf galaxies; gas accretion favours continual r-process enrichment in thes

126 d reveal the causal relationship between the accretion flow and the powerful jet emission.

127 suggests the presence of an outflow from the accretion flow onto the SMBH.

128 port observations that reveal a cold, clumpy accretion flow towards a supermassive black hole fuel re

129 minous filament, consistent with such a cold accretion flow, was discovered near the quasi-stellar ob

130 perties are strongly coupled to those of the accretion flow.

131 he geometry is strongly suggestive of a cold accretion flow.

132 hereby precluding a detailed analysis of the accretion flow.

133 Hydrodynamic simulations suggest that 'cold accretion flows'--relatively cool (temperatures of the o

134 und here is indicative of growth by coherent accretion for this black hole, and suggests that black-h

135 ertain whether the explosion is triggered by accretion from a non-degenerate companion star or by a m

136 the hypothesis that they arose by fusion and accretion from an ancestral set of peptides active as co

137 Early adiposity accretion from birth to 9 years and late linear growth f

138 (Fosl2), potentiates the rate of myocardial accretion from the zebrafish SHF.

139 Periodic variations consistent with pulsed accretion have been seen in only a few young binaries vi

140 lution of the Moon, and for testing the late-accretion hypothesis.

141 Accretion in microquasars varies on much shorter timesca

142 peak II (r=0.625( * *)), and decreased with accretion in peak I (r=-0.623( * *)).

143 with a change in ECM properties favors lipid accretion in tendons.

144 (176m)Lu, due to an irradiation event during accretion in the early solar system.

145 mechanism that can trigger supra-exponential accretion in the early universe, when a BH seed is bound

146 r growth in the first decade of life and fat accretion in the second decade are associated with adult

147 rsts of oral corticosteroids on bone mineral accretion in this regard.

148 implies the existence of magnetically gated accretion, in which disk material builds up around the m

149 e of steady background flow and limited mass accretion indicating significant mechanical nonlinearity

150 the capacity of batroxobin to promote fibrin accretion is 18-fold greater than that of thrombin, a fi

151 Progressive structure accretion is observed for the peptide in water, LPS, and

152 are thought to grow mostly by merger-driven accretion leading to high spin.

153 the inner disk (around GG Tau Aa) beyond the accretion lifetime, leaving time for planet formation to

154 The accretion light curve is modulated over the binary orbit

155 ly late (hundreds of millions of years after accretion), long-lasting, intense and widespread epoch o

156 ccretion tracers, albeit intermittently with accretion luminosity variations ranging from zero to 50

157 with the protoplanetary disk through chaotic accretion , magnetic interactions or torques from neighb

158 To sustain mineral accretion, maturation ameloblasts need to buffer these p

159 nces in adipokines and myocardial fatty acid accretion may underlie heterogeneous data from rodent st

160 w insights into nacre formation and particle-accretion mechanisms that may be common to many calcareo

161 sence of an unstable, magnetically regulated accretion mode, which in turn implies the existence of m

162 ula gas dissipated, consistent with the core accretion model for giant planet formation.

163 The survey measurements support the core accretion model, in which planets form by the accumulati

164 In this Accretion Model, small RNAs and peptides were subsumed o

165 ular clouds--a departure from the 'hot mode' accretion model--although unambiguous observational supp

166 Standard accretion models fail to explain its luminosity, even as

167 The lack of sustained accretion--not the actual rate--would then be the critic

168 Biodistribution studies revealed accretion of (89)Zr-DFO-mAb-B43.13 in the OVCAR3 tumors,

169 depletion may be explained qualitatively by accretion of 10 to 20 per cent of a volatile-rich body t

170 n of membranes and not simply COPII-mediated accretion of a larger surface of ER.

171 e of radiation from the tidal disruption and accretion of a star can be used as a marker for supermas

172 s that the role of the magnetic field in the accretion of a T Tauri star is more complex than our cur

173 ing and vaporization rather than with simple accretion of a volatile-rich chondrite-like body.

174 the diffuse biomat (i.e., 80 +/- 20%), with accretion of assimilated nitrogen accounting for less th

175 on the early Earth could have benefited from accretion of carbonaceous meteorites both directly with

176 Cooling can be regulated by feedback from accretion of cooling gas onto the central black hole, bu

177 f planetary formation by mediating the rapid accretion of disk material onto the central star and the

178 Accretion of domains and molecules gave rise to modern a

179 esis and crustal shortening, coincident with accretion of exotic crust.

180 1) are thought to be powered by the accretion of gas onto black holes with masses of approxi

181 1); ref. 1) are thought to be powered by the accretion of gas onto black holes with masses of approxi

182 lack holes in galaxy centres can grow by the accretion of gas, liberating energy that might regulate

183 efore, in addition to late-stage terrestrial accretion of halogens and mantle degassing, which has re

184 We propose that TANGO1/cTAGE5 promotes the accretion of inner coat proteins to the helical lattice.

185 ese differences were attributable to greater accretion of lean mass, rather than fat mass.

186 Simple models involving the gradual outboard accretion of material along curvilinear subduction zones

187 asars are associated with and powered by the accretion of material onto massive black holes; the dete

188 Accretion of matter onto black holes is universally asso

189 n, and it challenges physical models for the accretion of matter onto magnetized compact objects.

190 was of interest to determine how this large accretion of mobile elements affects competitive growth

191 of multidrug-resistant enterococci: (i) the accretion of mobile elements in E. faecalis V583 renders

192 The Earth formed by accretion of Moon- to Mars-size embryos coming from vari

193 neonatal muscle growth results from nuclear accretion of myoblasts preferentially at the tips of myo

194 These results suggest that net accretion of outer barrier reef communities will decline

195 hat accumulation of flavonols alleviated the accretion of reactive oxygen species during abiotic stre

196 ise and to avoid inundation through vertical accretion of sediments, which allows them to maintain we

197 extent to which they affect the behavior and accretion of senescent cells within distinct tissues is

198 earrangement and three-dimensional growth by accretion of silica molecules.

199 ontinuously through hierarchical merging and accretion of smaller systems.

200 fire-prone, summer-dry climates or sustained accretion of species under inferred stable climate regim

201 Although such rapid accretion of the gas-giant cores has successfully been m

202 -(53)Cr ages of aqueous alteration, suggests accretion of the L, CV and CO parent bodies approximatel

203 ophes occurred in our solar system since the accretion of the planets.

204 e Earth ratio therefore is best satisfied by accretion of thermally processed objects followed by lar

205 bilitated with cafeteria formula had greater accretion of visceral than subcutaneous fat, showed incr

206 e the melting processes that occurred during accretion on Earth and precursor bodies and report vapor

207 ades of life the higher the adult BP; linear accretion only in the first decade of life was associate

208 They are thought to be powered by accretion onto a compact object.

209 wn, perhaps during the quasar phase of rapid accretion onto a supermassive black hole, an unknown mec

210 ough a hyperluminous quasar phase powered by accretion onto a supermassive black hole.

211 a fundamental ingredient in regulating mass accretion onto black holes.

212 c nuclei (AGN) shone brightly as a result of accretion onto black holes.

213 per second can be explained by supercritical accretion onto massive stellar-mass black holes.

214 Possible explanations include accretion onto neutron stars with strong magnetic fields

215 Attempts to observe directly signatures of accretion onto protoplanets have hitherto proven unsucce

216 Given that the inner disks are depleted by accretion onto the stars on timescales of a few thousand

217 e dwarfs and extends the connections between accretion onto white dwarfs, young stellar objects and n

218 ese black holes continue to grow by coherent accretion or in a chaotic manner, though clear differenc

219 ons of planetary bodies are a consequence of accretion or inherited from prior nebular fractionation.

220 ed independent of length as FFM index (FFMI) accretion over 12 weeks.

221 During the peak of their accretion phase, supermassive black holes in galactic co

222 The luminous, but brief, accretion phases shown by transients with large accretio

223 providing constraints on physical models of accretion physics in black hole and neutron star binary

224 to be consistent with the "cold-start" core-accretion process that may have formed Jupiter.

225 is an important parameter of the black hole accretion process.

226 s a reliable tool to predict the erosion and accretion processes controlling the evolution of small s

227 Although generally associated with the accretion processes necessary for marshes to keep up wit

228 etion disk demonstrates a connection between accretion processes occurring on very different scales:

229 These accretion processes respond to changes in local and glob

230 es may directly or indirectly influence soil accretion processes through the production and accumulat

231 eory performs well for 2-methyltetrols, once accretion product decomposition is taken into account.

232 OA) is derived from thermal decomposition of accretion products or other low volatility organics havi

233 s may be bound in low-volatility mass (e.g., accretion products, inorganic-organic adducts) that deco

234 The high gas opacity traps the accretion radiation, while the low-mass BH's random moti

235 b weight, linear growth rate, muscle protein accretion rate and fractional synthetic rate were lower

236 a high-resolution 3,000 year record of reef accretion rate and herbivore (parrotfish and urchin) abu

237 onto the central black hole, but requires an accretion rate finely tuned to the thermodynamic state o

238 This suggests that the accretion rate is not the critical parameter for inducin

239 The switch increased the reef's accretion rate, allowing it to keep pace with rising sea

240 en observed only in sources with a high mass-accretion rate, such as GRS 1915+105.

241 state of which depends primarily on the mass-accretion rate.

242 ity arising from a temporary increase in the accretion rate.

243 estimate broad properties, such as the mass accretion rate.

244 bol derived by assuming an Eddington-limited accretion rate.

245 r 1.5 My, possibly due to a drop in the disk accretion rate.

246 ack holes is therefore their mass-normalized accretion rate.

247 Calculated accretion rates (mm year(-1)) for shallow fore-reef habi

248 At each site, declines in accretion rates and parrotfish abundance were initiated

249 s using convergent cross mapping reveal that accretion rates are driven by parrotfish abundance (but

250 f the circumnuclear material with increasing accretion rates has been found by studies across the ele

251 ncreases in luminosity arising from variable accretion rates have been predicted for some pre-main-se

252 imb blood flow, substrate uptake and protein accretion rates in skeletal muscle, late gestation contr

253 f 100 seconds to 2.5 hours can occur at mass-accretion rates more than ten times lower than previousl

254 Comparison of vertical accretion rates with RSLR rates at the land surface (pre

255 The anomalously high accretion rates, obtained using (14)C age dating, were c

256 h are identical but for their widely varying accretion rates-has been a longstanding puzzle.

257 c volatile organic compounds (BVOCs) through accretion reactions and organosulfate formation.

258 ugh condensation, while dimers are formed by accretion reactions within the particle phase as the par

259 In this model, the ribosome evolved by accretion, recursively adding expansion segments, iterat

260 ss, which suggested that a poor bone mineral accretion reflected poor growth.

261 ules and their significance for planetesimal accretion remain enigmatic.

262 initiation, rate and duration of myocardial accretion remain obscure.

263 After that the nova awakes again-with accretion returning to the pre-eruption level and leadin

264 that these cold clouds also fuel black hole accretion, revealing 'shadows' cast by the molecular clo

265 een nascent envelopes and young disks due to accretion shocks.

266 The strength and regularity of this accretion signal is surprising; it may be related to the

267 ng the class 0 protostellar phase (the early accretion stage), and continue during the subsequent cla

268 els of the prevalent radiatively inefficient accretion state.

269 of the source present a natural analogy with accretion-state changes of stellar mass black holes, whi

270 Accretion stops, and the pre-main sequence star that eme

271 l influences controlling elevation (sediment accretion, subsidence), mangrove replacement of salt mar

272 together with an absence of obvious signs of accretion, suggests that AR Sco is primarily spin-powere

273 ere it contributes 2-5 times more to surface accretion than an equal mass of minerals.

274 97 kg/m2 (95% CI -0.002, 0.196) greater FFMI accretion than having 0% milk protein, although this dif

275 icant departures from the standard thin disk accretion that powers bright Galactic X-ray binaries, or

276 This model is known as 'pebble accretion'; theoretically, it can produce cores of ten E

277 This is in good agreement with the core-accretion theory of planet formation, in which a gas gia

278 Core-accretion theory predicts that, given the small masses o

279 ), increased rates of SLR would outpace reef accretion, thereby reducing the depth range of substrate

280 on chondrite parent bodies constrains their accretion times and thermal histories.

281 ng the first five million years of planetary accretion to explain their observed abundance.

282 ted to shift coral reefs from a state of net accretion to one of net dissolution this century.

283 diverged as a result of disproportional late accretion to the Earth and Moon.

284 densities too low to maintain sustained mass accretion to the inner part of the disk.

285 The timing of water accretion to the inner solar system also has implication

286 een in only a few young binaries via optical accretion tracers, albeit intermittently with accretion

287 ting incident storm wave energy and, through accretion, tracking increasing water depths consequent u

288 ent gas cloud, and it grows by sporadic mass accretion until it acquires 34,000 solar masses.

289 Accretion variability is a common feature of young stars

290 s, vegetation type had no effect on rates of accretion, vertical movement in root and sub-root zones,

291 t was held constant by preventing myonuclear accretion via satellite cell depletion, both the number

292 a new model called Viscously Stirred Pebble Accretion (VSPA) has been developed that can explain the

293 compared to children who received CSB, FFMI accretion was increased by 0.083 kg/m2 (95% CI 0.003, 0.

294 Since planetary accretion, water has been exchanged between the hydrosph

295 ponse to IGF-1, myotube diameter and protein accretion were sustained.

296 a vicious cycle of cholesterol synthesis and accretion, which may cause gradual neurodegeneration, an

297 rect the myocardial deficit by extending the accretion window.

298 athway, and fibrogenesis despite similar fat accretion with diet-induced obesity.

299 ng the origin of water and the timing of its accretion within the inner solar system is important for

300 le Ru record different stages of the Earth's accretion; yet all those elements point to material that