ライフサイエンスコーパス: merger

1 Ypt7 needed for SNARE-mediated lipid bilayer merger.

2 onal-wave detection of a binary neutron-star merger.

3 ration tendency of PE to facilitate membrane merger.

4 e a general mechanism to drive lipid bilayer merger.

5 protein, which is also involved in membrane merger.

6 , rate-limiting event that precedes membrane merger.

7 ble conformational changes to cause membrane merger.

8 nformational changes culminating in membrane merger.

9 ell membrane, enabling F to mediate membrane merger.

10 protein function until the onset of membrane merger.

11 lack hole systems inspiraling toward a final merger.

12 ps in the fusion process, ending in membrane merger.

13 pin conformations in the process of membrane merger.

14 conformational changes that lead to membrane merger.

15 nts show that HAP2 is essential for membrane merger.

16 sion (F) glycoprotein that mediates membrane merger.

17 nd archaeal cells that underwent a symbiotic merger.

18 ave remained stable overall since the genome merger.

19 dynamical instabilities and a possible eddy merger.

20 has been postulated to function in membrane merger.

21 agnose the energetics and environment of the merger.

22 7a from 11.75 hours until 8.5 days after the merger.

23 dictions of blue kilonovae from neutron-star mergers.

24 other possible sources, such as neutron star mergers.

25 -poor stars that were added during late-time mergers.

26 nly during rare events, such as neutron star mergers.

27 2 collisions, including both major and minor mergers.

28 ive black hole binaries formed during galaxy mergers.

29 feedback at earlier times, not through major mergers.

30 s currently thought) assembling entirely via mergers.

31 GW190425, both originating from neutron-star mergers.

32 and we also consider the possibility of firm mergers.

33 s of galaxies through accretion and repeated mergers.

34 ll departments or they have vanished through mergers.

35 of their mass by accretion rather than major mergers.

36 stars and the expected rate of neutron star mergers.

37 stellar metallicities than with neutron-star mergers.

38 o be detectable from lower-mass neutron-star mergers.

39 e a primary formation channel for black-hole mergers(11-13), but the rates and properties(14,15) of t

40 g through the accretion of cold material and mergers(3,4).

41 present formation channels of compact-object mergers(7).

42 ce for a causal link between gas-rich galaxy mergers, accretion onto the nuclear SMBH, and coeval sta

43 ogically associating domain (TAD) splits and mergers across the genome between Hi-C samples.

44 M algorithm) into edge-covering Quasi-Clique Merger algorithm (eQCM) for mining weighted sub-network

45 We modified the Quasi-Clique Merger algorithm (QCM algorithm) into edge-covering Quas

46 mation through either cold-mode accretion or mergers, although its large rotational velocity and larg

47 to these technologies and inciting increased merger and acquisition activity that has yielded signifi

48 rgenomic interactions that arise from genome merger and allopolyploidization.

49 Transcriptomic responses to genomic merger and doubling have been demonstrated in many allop

50 Our findings demonstrate that genomic merger and doubling have consequences that extend beyond

51 Genomic merger and doubling induce an extensive array of genomic

52 begins with the earliest responses to genome merger and doubling; less is known about chromosomal dip

53 omparisons of the diverse outcomes of genome merger and duplication on abiotic niche preference.

54 of repeat-associated siRNAs following genome merger and genome duplication in the context of allopoly

55 rential expression patterns following genome merger and genome duplication.

56 at simulates gene genealogies under multiple merger and Kingman's coalescent processes within species

57 Membrane merger and pore formation were also examined.

58 Motivated by the merger and redesign of these long-standing HIV cohort st

59 in the orbit, but the former would lead to a merger and the latter to an overluminous companion.

60 of the mass ejection associated with such a merger and the subsequent evolution of the ejecta, and w

61 ional rearrangements to bring about membrane merger and virus entry.

62 enuating misregulation resulting from genome merger and/or doubling.

63 ission after discharge) and data on hospital mergers and acquisitions occurring from 2009 through 201

64 ing the connection between binary black hole mergers and active galactic nuclei as hosts, even if onl

65 ystems are an expected consequence of galaxy mergers and can provide important constraints on models

66 ly accreted from either stellar mass loss or mergers and that would otherwise cool to form stars.

67 ered with the detection of binary black-hole mergers and they should also be detectable from lower-ma

68 a-relativistic jet being launched during the merger (and successfully breaking out of the surrounding

69 System point to their origin in neutron-star mergers, and indicate substantial deposition by a single

70 origin of r-process elements in neutron-star mergers, and shows that neutron stars are made of neutro

71 Stellar mergers are a brief but common phase in the evolution of

72 rate inferred from GW170817 imply that such mergers are a dominant mode of r-process production in t

73 om increased market power following hospital mergers are passed onto payers and consumers as lower co

74 evidence indicates that binary neutron-star mergers are the primary origin of heavy elements produce

75 orrect, then it confirms that compact-object mergers are the progenitors of short-duration gamma-ray

76 Whereas such multiple mergers are unlikely under the neutral coalescent, they

77 Kulkarni et al. suggest an exotic stellar merger as the possible origin.

78 umstantial evidence(6) point to neutron-star mergers as a probable r-process site; the optical/infrar

79 redicted from models that posit neutron-star mergers as the drivers of short hard-gamma-ray bursts.

80 1 provides a look at an unobstructed stellar merger at an evolutionary stage between its dynamic onse

81 to switch between different types of lineage mergers at run-time or even compile-time.

82 arch suggests that eukaryotes evolved from a merger between a host of archaeal descent and an alphapr

83 It is found that the probability of merger between bigger firms is bigger than that between

84 canonical insect tra-dsx pathway evolved via merger between expanding dsx function (from males to bot

85 t step of this process is represented by the merger between the vesicle and the plasma membranes, and

86 We propose that haemagglutinin induces a merger between the viral and target membranes by one of

87 show that we are observing the remnant of a merger between two dwarf galaxies.

88 e model predictions by observing dynamics of merger between two M. xanthus strains, where one strain

89 Its anomalies have long been attributed to a merger between two massive stars that occurred some 20,0

90 star formation are believed to be driven by mergers between gas-rich galaxies.

91 lyses and defines hundreds of TAD splits and mergers between pairs of different cell types, such as e

92 he different C++ highly reusable coalescence mergers (binary, multiple, hybrids) are given, and we il

93 ion is not concomitant with immediate genome merger, but occurs within the first generations of allop

94 observations, performed 207.4 days after the merger by using a global network of 32 radio telescopes.

95 al waves from stellar-mass binary black hole mergers by the Laser Interferometer Gravitational-wave O

96 istically less significant binary black hole merger candidate LVT151012.

97 re, we draw particular attention to multiple-merger coalescent events and background selection, discu

98 Because multiple merger coalescents emerge in many models of rapid adapta

99 pstakes reproduction and associated multiple-merger coalescents will become at least as relevant as t

100 t shows a similar, but less severe, membrane merger defect as a DeltaPrm1 mutant.

101 embrane domains (TMDs) in promoting membrane merger (Dhara et al., 2016), the underlying mechanism re

102 s in bulges grow rapidly to high masses when mergers drive gas infall that feeds quasar-like events.

103 ve black holes are thought to grow mostly by merger-driven accretion leading to high spin.

104 must have formed in a disk, rather than in a merger-driven nuclear starburst.

105 evelopment, molecular mechanisms of membrane merger during cell-cell fusion in most eukaryotic organi

106 rison with spectral models suggests that the merger ejected 0.03 to 0.05 solar masses of material, in

107 The binary neutron star merger event GW170817 was detected through both electrom

108 ave been detected from a binary neutron star merger event, GW170817.

109 nct phases that result from a massive galaxy merger event.

110 te substantial deposition by a single nearby merger event.

111 ificant number of multiple- and simultaneous-merger events under the DTWF model, which are absent in

112 s suggests that they are the result of minor merger evolution.

113 d by nucleosynthesis that occurs in the post-merger fast-moving dynamical ejecta and in two slower (0

114 ein fusion machineries that mediate membrane merger for infection.

115 iquitous phenomenon produced in neutron-star mergers, giving rise to a hitherto unidentified populati

116 avitational waves from two binary black hole mergers, GW150914 and GW151226, along with the statistic

117 following the discovery of the neutron-star merger GW170817 by gravitational-wave detectors(10)-was

118 nova associated with the binary neutron-star merger GW170817 remains the only confirmed electromagnet

119 he EM counterpart of the binary neutron star merger GW170817.

120 Ws) were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ra

121 s (GWs) emanating from a binary neutron star merger, GW170817.

122 Although a handful of stellar mergers have been observed directly(8,9), the central re

123 Multiple studies have shown that hospital mergers have led to higher prices for commercially insur

124 ry black hole observations.Binary black hole mergers have recently been observed through the detectio

125 ups that are associated with either membrane merger (hemifusion) or fusion pore expansion.

126 as by the accidents of its recent haphazard merger history.

127 A complete picture of compact object mergers, however, requires the detection of an electroma

128 The merger hypothesis is further supported by a lack of magn

129 rotein machinery that drives plasma-membrane merger in different systems, which is characterized by d

130 hat it is the product of a gentle, low-speed merger in the early Solar System.

131 ce GW170817 arose from a binary neutron-star merger in the nearby Universe with a relatively well con

132 adial position suggest that mass transfer or mergers in binary stars dominates the production of blue

133 Mergers in hierarchical triple stars are marginally perm

134 o perform dynamic analysis of TAD splits and mergers in numerous biological and disease models.

135 The role of mergers in producing galaxies, together with the finding

136 we implement several variants of coalescent mergers, including an approximation where low probabilit

137 erium Myxococcus xanthus to show that colony-merger incompatibilities can be strong barriers to socia

138 ributing factors resulting from the numerous mergers, increase in out-sourcing, and the heavy depende

139 e looking forward to the detection of binary mergers involving neutron stars and their electromagneti

140 'kilonova' that emerges in the days after a merger is a likely place to detect the spectral signatur

141 mechanisms with which gp41 induces membrane merger is limited by the fact that the hydrophobic N-ter

142 sters; our predicted detection rate of these mergers is comparable to that from homogeneous evolution

143 neutron capture (r-process) in neutron-star mergers is expected theoretically and is supported by mu

144 astic confusion background of compact-object mergers, known sources detected in unexpected ways, and

145 mass spiral galaxies in this evolution; such mergers lead to an elliptical galaxy, as in the case of

146 e of budding domains, but broadened by their merger, matched the virus size distribution.

147 Selective membrane mergers may be driven by small-molecule recognition betw

148 We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, someti

149 ay transients powered by binary neutron-star mergers may not be associated with a short gamma-ray bur

150 the expectations from standard neutron-star merger models.

151 As neutron-star mergers occur infrequently, their deposition of radioact

152 tion from the same source has shown that the merger occurred in the outskirts of the galaxy NGC 4993,

153 The productive merger of a chiral imidazolidinone organocatalyst and a

154 The productive merger of a thiol catalyst and a commercially available

155 conjugate (general structure 7) embodies the merger of a very potent and proven anabolic selective ag

156 trongly indicates that gene fusions arose by merger of adjacent open reading frames.

157 This process is enabled by the merger of aerobic oxidative Cu-catalysis with decarboxyl

158 hat these three supernovae resulted from the merger of binary white dwarfs or other compact stars suc

159 medical realm has led to a highly productive merger of clinical, experimental and environmental micro

160 riencing a comeback, enabled by the powerful merger of detailed mechanistic studies and systems-level

161 gene clusters on similar phenotypes and the merger of distinct gene clusters into a single functiona

162 of expression evolution accompanying genomic merger of divergent diploid parents, genome doubling, an

163 Particularly, the merger of Earth-abundant 3d metal catalysis and electroo

164 redictions provide a promising arena for the merger of economics and biology [1-6].

165 cept is exemplified by MacMillan's beautiful merger of enamine and iminium ion activation, examples i

166 on a viral glycoprotein, Gc, to catalyze the merger of endosomal host and viral membranes during cell

167 octoploid species, both descendants from the merger of four diploid progenitor species into a single

168 ionalization (DCF) of olefins enabled by the merger of Giese-type addition with Ni/photoredox dual ca

169 delayed, possibly because colocalization and merger of ICP0 with nuclear bodies containing Sp100 and

170 The reaction is driven by a merger of iminium catalysis and redox activity of the co

171 le cloud collapse followed by a low-velocity merger of its two lobes.

172 C(sp(3))-H trifluoromethylation through the merger of light-driven, decatungstate-catalysed hydrogen

173 ential step in the nucleation is the initial merger of lipid headgroups at the nascent pore center.

174 dergo cell-cell recognition and adhesion and merger of membranes between apposing cells.

175 Such a merger of microfluidics with biosensing technologies all

176 mitting graphical specification of rules and merger of networks generated automatically (using the Bi

177 A merger of new and published results leads to a new model

178 atalytic strategy has been developed via the merger of NHC and H-bonding catalysis.

179 chemistry has seen major advances due to the merger of nickel and photoredox catalysis.

180 This was achieved by the successful merger of palladium-catalyzed C-H functionalization and

181 The merger of PDA imprinting with dynamic functionalized ves

182 lly useful asymmetric transformations by the merger of photocatalysis and enzyme catalysis.

183 resents the oxygenation of C-H bonds via the merger of photocatalysis and Pd catalysis.

184 ing of arylboronic acids with CF(3)I via the merger of photoredox and Cu catalysis.

185 lating reagents, achieved via the successful merger of photoredox and hydrogen atom transfer catalysi

186 Here we demonstrate that the synergistic merger of photoredox and nickel catalysis enables the di

187 The merger of photoredox and nickel catalysis has enabled th

188 Using this synergistic merger of photoredox and nickel catalysis, we have devel

189 upling has been achieved via the synergistic merger of photoredox and nickel catalysis.

190 as been accomplished through the synergistic merger of photoredox and nickel catalysis.

191 trophile coupling has been developed via the merger of photoredox and transition metal catalysis.

192 zation has been achieved via the synergistic merger of photoredox, nickel, and hydrogen atom transfer

193 ntial for sexual reproduction and exoplasmic merger of plasma membranes.

194 Through the merger of previously independent lineages, symbiosis pro

195 s through distinct steps, including docking, merger of proximal leaflets (stalk formation), and forma

196 The approach entails the merger of several catalytic processes and is expected to

197 elayed B-cell contraction, inhibition in the merger of signaling active BCR microclusters into signal

198 r the fluorination of alkyl bromides via the merger of silyl radical-mediated halogen-atom abstractio

199 olecules often evolve through the successive merger of smaller sub-clusters, which function as indepe

200 e cooperative lipid tilting, leading to self-merger of the inner monolayer of NT (hemifission), consi

201 embrane adhesion, presumably directly in the merger of the lipid bilayers.

202 The merger of the Pediatric Oncology Group, Children's Cance

203 The merger of the RPTC model and multiwell respirometry resu

204 lease, i.e., fusion pore formation after the merger of the two lipid membranes occurs almost simultan

205 es using individual data sources or a simple merger of the two.

206 on-mediating glycoproteins to facilitate the merger of the viral and host cell membranes.

207 post-fusion state, a process that drives the merger of the viral and host cell membranes.

208 Viral fusogens mediate the merger of the viral envelope and cellular membrane durin

209 ction of cells by enveloped viruses requires merger of the viral envelope membrane with target cell m

210 ng of the fusion (F) protein, which leads to merger of the viral envelope with target cell membranes.

211 Viral fusion proteins catalyze the merger of the virus envelope and the target cell membran

212 allowed for survival after WGD, and that the merger of these species is greater than the sum of their

213 Here we report the merger of these two devices: the light-emitting electroc

214 The merger of these two modes of catalysis leverages nickel'

215 -item lists, linking did not yield immediate merger of three 15-item lists into a 45-item list, altho

216 Here, we show that the synergistic merger of three catalytic processes-photoredox, enamine

217 he semifertile triploid hybrid can promote a merger of three different genomes and demonstrate how im

218 We found that initial merger of two cell membranes detected as lipid mixing in

219 ndicate that GW170817 is consistent with the merger of two compact objects, the electromagnetic obser

220 roduced by a relativistic jet created by the merger of two compact stellar objects (specifically two

221 f membrane proteins that drive the efficient merger of two distinct lipid bilayers into one interconn

222 of insect wings (that is, novelty through a merger of two distinct tissues).

223 ession level dominance accompany the initial merger of two diverged diploid genomes, suggesting a com

224 The merger of two gametes is achieved through a two-step mec

225 The merger of two highly utilized and robust catalytic syste

226 Through the unprecedented merger of two independent, yet complementary, catalysis

227 t of lipids and proteins that results in the merger of two lipid bilayers.

228 The merger of two massive (about 30 solar masses) black hole

229 ength high-resolution observations of a rare merger of two massive submillimetre bright galaxies at z

230 t the matter that is expelled in the violent merger of two neutron stars can assemble into heavy elem

231 The merger of two neutron stars is predicted to give rise to

232 We report a study involving the successful merger of two separate chiral catalytic cycles: a chiral

233 CK Vul is best explained as the remnant of a merger of two stars.

234 The explosion could be triggered by the merger of two white dwarfs (a 'double-degenerate' origin

235 Exocytosis, consisting of the merger of vesicle and plasma membrane, is a common mecha

236 Minor mergers of a spiral galaxy with a smaller companion shou

237 st in coalescent models which admit multiple mergers of ancestral lineages; and to model hybridizatio

238 embled from smaller pieces, through numerous mergers of cold dark matter.

239 nuclei) demonstrate the importance of major mergers of equal-mass spiral galaxies in this evolution;

240 t mode by which galaxies grow, because major mergers of galaxies would completely disrupt the observe

241 Mergers of lower-mass galaxies are expected within the h

242 show that a simple physical model describing mergers of massive, gas-rich galaxies matches these obse

243 Mergers of neutron stars are known to be associated with

244 such as magnetars over models involving the mergers of older neutron stars, which are more likely to

245 TADsplimer recaptures splits and mergers of TADs with high accuracy in simulation analyse

246 pid kinetics of the sequential and separable mergers of the outer and inner membranes, but allowed on

247 Mergers of this kind are also expected to create signifi

248 servoirs, which could be provided by ongoing mergers or cold-stream accretion.

249 of non-thermal electrons produced by cluster mergers or injected by radio galaxy jets, which impacts

250 formation processes, such as mass transfer, mergers or stellar collisions during dynamical encounter

251 rial that was ejected dynamically during the merger, or a cocoon of material that breaks out when a j

252 i as hosts, even if only a sub-population of mergers originate from active galactic nuclei.

253 one stage of cotton development, that genome merger per se has a large effect on relative expression

254 predict detections of about 1,000 black-hole mergers per year with total masses of 20-80 solar masses

255 vy elements, demonstrating that neutron star mergers play a role in rapid neutron capture (r-process)

256 Mergers play an important role in galaxy evolution and a

257 rienced angular momentum loss and subsequent merger, possibly because of dynamical friction and colli

258 ly secular in origin and that low-mass minor mergers predicted to be common throughout the Universe p

259 This indicates that neutron-star mergers produce gravitational waves and radioactively po

260 close binaries(8,9), which is as expected if mergers produce magnetic stars.

261 tions show that at least 10% of neutron star mergers produce such a jet.

262 Galaxy mergers produce supermassive black hole binaries, which

263 gnetic observations of a double neutron star merger producing gravitational waves led to a focus on m

264 The ejected mass and a merger rate inferred from GW170817 imply that such merge

265 The merger rate of bronchial asthma of the patients seen in

266 with observational estimates of neutron-star merger rates(6-8), but rules out supernovae and stellar

267 S17a was the result of a binary neutron star merger, reinforcing the gravitational wave result.

268 egimes of interest: layer-forming splats and mergers resulting in bilobed shapes.

269 ervations with current theoretical models of mergers suggests that they are the result of minor merge

270 proximately 40 times more binary-black-holes mergers than do dynamical formation channels involving g

271 find that there was probably a single nearby merger that produced much of the curium and a substantia

272 or a time, ultimately undergoing a low-speed merger that will result in a new bilobate configuration.

273 found our efforts to reconstruct the ancient mergers that forged multiple lines of photosynthetic mic

274 he event-rate density of binary neutron-star mergers that is robustly inferred from the detection of

275 n on purely baryonic processes in the galaxy mergers that make bulges.

276 Within 100 days of the merger, the radio light curves will enable observers to

277 ly, 5-90 s) after the sample/reagent droplet merger, the volume of the released gas scales with the a

278 these supernovae are rarer than neutron-star mergers, the larger amount of material ejected per event

279 ion have recently culminated in a successful merger: the development and clinical application of gene

280 l dominance increases over time, from genome merger through evolution at the polyploid level.

281 irus parainfluenza virus 5 mediates membrane merger through its fusion protein (F).

282 sion networks and local maximal quasi-clique merger to identify gene co-expression modules.

283 on with multiple parameter settings and data merger to optimize the balance between sensitivity and r

284 there has been no conclusive proof that this merger took place.

285 at breaks out when a jet launched during the merger transfers its energy to the dynamical ejecta.

286 l surface mediated hemifusion (outer leaflet merger) upon low-pH treatment, but only those containing

287 y and tightly docked state preceding leaflet merger using arresting point mutations in SNARE proteins

288 ulatory mismatches caused by initial genomic merger, while new gene expression conditions are generat

289 Such a merger will elucidate the genetic basis of adaptive beha

290 Probing the origin of binary black hole mergers will be difficult due to the expected lack of el

291 s the density increases), at least some such mergers will leave behind a supramassive or even a stabl

292 within its lipid bilayer to mediate membrane merger with a cell membrane for entry.

293 lar iodo halo-Michael aldol reaction and its merger with an ABCD ring fragment to afford the congener

294 from a non-degenerate companion star or by a merger with another white dwarf.

295 the protein to the virus envelope during its merger with the cell membrane.

296 Since vesicle membrane merger with the plasma membrane is reflected in plasma m

297 Observations of neutron-star mergers with distinct messengers, including gravitationa

298 We conclude that gas-rich major galaxy mergers with intense star formation can form the most ma

299 ocal elliptical galaxies seen today, through mergers with minor companions, but validating this pictu

300 A merger would also ensue if mass transfer to the black ho