ライフサイエンスコーパス: dwarf

1 n 2,700 kelvin are referred to as 'ultracool dwarfs'.

2 led onto a highly magnetized (B>10 MG) white dwarf.

3 anion star or by a merger with another white dwarf.

4 ements for the precursor to a low-mass white dwarf.

5 hite dwarf merging with a less-massive white dwarf.

6 aints that suggest that the donor is a brown dwarf.

7 onuclear runaway on the surface of the white dwarf.

8 nse plasma related to the viscosity of brown dwarfs.

9 estructive explosions of carbon-oxygen white dwarfs.

10 isk instabilities drop matter onto the white dwarfs.

11 e of the weather phenomena reported on brown dwarfs.

12 erate objects, either neutron stars or white dwarfs.

13 n evolved stars, in dust clouds and on brown dwarfs.

14 d F-type stars that end their lives as white dwarfs.

15 t high rates of mass transfer to their white dwarfs.

16 al peaks of rotavirus and all-cause AGE were dwarfed.

17 ID1c silencing corresponded to the degree of dwarfing.

18 Conversely, LOH2 overexpression resulted in dwarfing.

19 ized to understand the mechanisms underlying dwarfing.

20 otypes, including spontaneous cell death and dwarfing.

21 ication of two new mutant alleles of TWISTED DWARF 1 (TWD1), twd1-4, and twd1-5.

22 equires the hormone-dependent interaction of DWARF 14 (D14), a probable candidate SL receptor, with D

23 Among the 26 genes deleted in hebiba, DWARF 14 LIKE is, the one responsible for loss of symbio

24 of 10to10 in models of the bright T4.5 brown dwarf 2MASS 0559-14 leads to significantly better agreem

25 D14), a probable candidate SL receptor, with DWARF 3 (D3), an F-box component of the Skp-Cullin-F-box

26 Here we show that DWARF 53 (D53) acts as a repressor of SL signalling and

27 nt SL-insensitive rice (Oryza sativa) mutant dwarf 53 (d53) and the cloning of D53, which encodes a s

28 accretion column onto the poles of the white dwarf, a star subclass known as AM Herculis.

29 vae are one type of outburst: when the white dwarf accretes enough matter from its companion, the res

30 egenerate channel, hypothesizes that a white dwarf accretes matter from a companion star and the resu

31 t that SN 2012Z was the explosion of a white dwarf accreting material from a helium-star companion.

32 Most stars become white dwarfs after they have exhausted their nuclear fuel (the

33 ion lines of M. truncatula results in severe dwarfing, altered development, reduction in lignin conte

34 d methylation changes are suppressed in Ames dwarf and calorie restricted mice and more selectively a

35 tolerance-conferring transcription factors, DWARF AND DELAYED FLOWERING1 (DDF1) and DDF2, that dupli

36 Under in vivo conditions, the dwarf and early senescence phenotypes of the mutant rema

37 t influences the lifespan of long-lived Ames dwarf and normal littermate control mice in a genotype a

38 protein TWISTED DWARF1 (FKBP42/TWD1) causes dwarf and twisted-organ phenotypes in Arabidopsis.

39 K3 in Arabidopsis thalianaCA-MPK3 plants are dwarfed and display a massive derepression of defense ge

40 HMWKO mice were not dwarfed and had significantly increased bone mineral den

41 As a result, ERF6 gain-of-function lines are dwarfed and hypersensitive to osmotic stress, while the

42 true knock-out mutants of MPK1 were severely dwarfed and sterile, and homozygous mpk1 seeds from hete

43 tive transcriptional process responsible for dwarfing and inhibition of lignin biosynthesis, and sugg

44 modifications are often also associated with dwarfing and other changes in plant growth.

45 will help to constrain the physics of white dwarfs and binary star evolution.

46 te characterizations of atmospheres of brown dwarfs and exoplanets, especially when observed in the n

47 lution of magnetic fields in accreting white dwarfs and extends the connections between accretion ont

48 ing they bridge the gap between hotter brown dwarfs and gas-giant planets.

49 The state and evolution of planets, brown dwarfs and neutron star crusts is determined by the prop

50 ism has been studied in the context of white dwarfs and type Ia supernovae, but hitherto was not cons

51 efs 7, 8; with a millisecond pulsar, a white dwarf, and a planetary-mass object in an orbit of severa

52 OID-6-OXIDASE, CONSTITUTIVE PHOTOMORPHOGENIC DWARF, and DIMINUTO) and one brassinosteroid-signaling g

53 a rocky planet, the maximum mass of a white dwarf, and the mass of a typical galaxy.

54 ems in which one star of the pair is a white dwarf, and which often generate bright and energetic ste

55 s are not expected to be launched from white dwarfs, and an origin from a black hole or a neutron sta

56 ic fields are more common amongst cool white dwarfs, and implies that the currently accepted ages of

57 t, given the small masses of these ultracool dwarfs, and the small sizes of their protoplanetary disk

58 effects, including but not limited to severe dwarfing appearance, chlorosis, nearly complete reductio

59 eskimo1-5 (esk1-5) is a dwarf Arabidopsis (Arabidopsis thaliana) mutant that has

60 radiation and the internal energy of a brown dwarf are comparable.

61 White dwarfs are compact stars, similar in size to Earth but a

62 Brown dwarfs are massive analogs of extrasolar giant planets a

63 Dynamical mass estimates show that many such dwarfs are more massive than expected from their luminos

64 White dwarfs are often found in binary systems with orbital pe

65 However, even in binaries, white dwarfs are rarely detected at far-infrared or radio freq

66 f heavy elements in the atmospheres of white dwarfs are similar to the ratios in rocky bodies in the

67 tly accepted ages of strongly magnetic white dwarfs are systematically too young.

68 tood, so the potential use of low-mass white dwarfs as independent clocks with which to test the spin

69 Mutation of KRP2 in a DELLA semi-dwarf background restored meristem size, but not stem gr

70 iated substellar donor in an accreting white-dwarf binary system.

71 lected across dominant groupings of species (dwarf birch shrubs, willow shrubs, other deciduous shrub

72 previously puzzling behaviors seen in brown dwarf brightness variations.

73 cl1 4cl2 and 4cl1 4cl2 4cl3 mutants are both dwarf but do not have further reduced lignin than the 4c

74 red orbiting Proxima Centauri, the closest M dwarf, but it probably does not transit and its true mas

75 thermonuclear runaway in carbon/oxygen white dwarfs, but it is uncertain whether the explosion is tri

76 zations was a relatively rare form of abuse, dwarfed by abuse by family members and other adults.

77 Financial support for protected areas is dwarfed by the benefits that they provide, but these ret

78 though the contamination of 4 mg/kg (Fe) was dwarfed by the intentional content of 5800 mg/kg (Fe as

79 further evidence that the pollution of white dwarfs by heavy elements might originate from disrupted

80 in close orbits with less dense stars, white dwarfs can strip material from their companions and the

81 the final decimal places) and the two white dwarf companions (0.19751(15)M[Symbol: see text] and 0.4

82 sources in globular clusters or ultracompact dwarf companions of parent elliptical galaxies.

83 oachondroplasia (PSACH), a severe short-limb dwarfing condition, results from mutations that cause mi

84 sulphur-doped plastic target heated to Brown Dwarf conditions by an ultra-intense laser.

85 Here we report the discovery of a white dwarf/cool star binary that emits from X-ray to radio wa

86 elling the properties of the cluster's white-dwarf cooling sequence.

87 otility and limb bone growth in West African Dwarf crocodiles, producing altered limb proportions whi

88 on in LER for a fast-growing ('K-31'), and a dwarf cultivar ('Bonsai') of tall fescue (Festuca arundi

89 These figures dwarf current, typically inadequate spending on conservi

90 Semi-dwarf DELLA mutants with improved harvest index and decr

91 edistribution in the atmosphere of the brown-dwarf donor.

92 able and the matter is dumped onto the white dwarf during quasi-periodic dwarf nova outbursts.

93 every 88.18 days, a long period for a white dwarf-eclipsing binary.

94 like SELlm (Mr 34.2 kDa) found in shoots of dwarf elder.

95 Isolated white dwarfs emit most of their power from ultraviolet to near

96 degenerate matter and lends support to white dwarf evolutionary theory.

97 n-sequence companion and ejecta from a white-dwarf explosion.

98 100-1,000 km above the surface of the white dwarf, far too small to be resolved with current telesco

99 extreme environments in which low-mass white dwarfs form cannot fully be exploited.

100 ight at the boundary between stars and brown dwarfs, from which we have detected radio and optical au

101 Ultra-compact dwarf galaxies are among the densest stellar systems in

102 ed compact elliptical and isolated quiescent dwarf galaxies are tidally stripped systems that ran awa

103 mically simpler, and more ancient ultrafaint dwarf galaxies assembled shortly after the first stars f

104 sters in the halo of the Milky Way formed in dwarf galaxies, as is commonly believed, then they were

105 ly known SLSNe-I that reside in star-forming dwarf galaxies, ASASSN-15lh appears to be hosted by a lu

106 ermassive black holes in other ultra-compact dwarf galaxies.

107 bserving the remnant of a merger between two dwarf galaxies.

108 e assumption that no gas accretes into those dwarf galaxies; gas accretion favours continual r-proces

109 The local dwarf galaxy I Zwicky 18, which has a metallicity about

110 e optics kinematic data of the ultra-compact dwarf galaxy M60-UCD1 that show a central velocity dispe

111 halos and the properties of the Milky Way's dwarf galaxy satellites.

112 A local dwarf galaxy, NGC 5253, has a young star cluster that pr

113 r than that detected in any other ultrafaint dwarf galaxy.

114 lyglutamine allele onto the slow-aging Snell dwarf genotype.

115 rocky, disintegrating bodies around a white dwarf have not yet been observed.

116 However, hitherto observations of brown dwarfs have been limited to globally integrated measurem

117 Between one-quarter and one-half of white dwarfs have elements heavier than helium in their atmosp

118 The coolest brown dwarfs have temperatures of 400 to 450 kelvin and masses

119 Recent results have shown that M dwarfs host Earth-sized planets in great numbers: the av

120 Since the observation of the first brown dwarf in 1995, numerous studies have led to a better und

121 terial accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclea

122 urface magnetic field strength for the white dwarf in MV Lyrae of between 2 x 10(4) gauss and 1 x 10(

123 ations of the 'non-magnetic' accreting white dwarf in the binary system MV Lyrae, whose light curve d

124 odel may account for the explosions of white dwarfs in a mass range wider than previously supposed.

125 also low, as in primeval galaxies and local dwarf irregular galaxies, CO forms slowly and is easily

126 observations of CO clouds in the local group dwarf irregular galaxy Wolf-Lundmark-Melotte (WLM), whic

127 he detection of CO in two regions of a local dwarf irregular galaxy, WLM, where the metallicity is 13

128 ensity explains why star clusters forming in dwarf irregulars have similar densities to star clusters

129 ear- and mid-infrared radiation if the white dwarf is magnetic.

130 se binaries, the magnetic field of the white dwarf is strong enough (at 10(6) gauss or more) to chann

131 aximum observed on high-field magnetic white dwarfs, is impossible because practically available fiel

132 es from stranded pygmy (Kogia breviceps) and dwarf (K. sima) sperm whales were used to characterize t

133 st rapid and well documented cases of island dwarfing known thus far took place over thousands of yea

134 y more massive population of accreting white dwarfs, large populations of low-mass X-ray binaries or

135 ified the causative mutation of the dominant dwarf Ligon lintless Li1 short fiber mutant as a single

136 very of a high proper motion, low-mass white dwarf (LP 40-365) that travels at a velocity greater tha

137 ve to weakly magnetic and non-magnetic white dwarfs, making them appear younger than they truly are.

138 Some dwarf male features are retained due to functional and m

139 Ghiselin noted that dwarf males are more common among smaller marine animals

140 sp. as a derived species, and the absence of dwarf males represents a character reversal for this gen

141 Harems of dwarf males reside in the lumen of the tube surrounding

142 We identified herbivory patterns in a dwarf mangrove forest on the archipelago of Twin Cays, B

143 the replication machinery of tobacco yellow dwarf mastrevirus (TYDV) and is essentially transient ge

144 dwarf, or on a sub-Chandrasekhar-mass white dwarf merging with a less-massive white dwarf.

145 o observed in the livers of long-lived Snell dwarf mice and in mice exposed to drugs that have been s

146 Compared with control mice, Snell dwarf mice exhibited differences in regional benzodiazep

147 hanisms responsible for reduced longevity of dwarf mice exposed to GH treatment early in life.

148 Studies in a separate cohort of Ames dwarf mice show that this short period of the GH exposur

149 Interestingly, in long-lived Ames dwarf mice, renal FXR and TGR5 expression levels were al

150 tly more slowly in bigenic HD knock-in/Snell dwarf mice.

151 were diminished in bigenic HD knock-in/Snell dwarf mice.

152 nificantly in male bigenic HD knock-in/Snell dwarf mice.

153 based experimental trials on habituated wild dwarf mongooses (Helogale parvula) [4], we combine sound

154 migration in a habituated population of wild dwarf mongooses (Helogale parvula) [5]; sentinels (raise

155 (SCMV) is the most important cause of maize dwarf mosaic disease.

156 ression on the cell-to-cell movement of Bean dwarf mosaic virus, a single-stranded DNA virus.

157 -TAG using the growth hormone-deficient Ames dwarf mouse model, which has reduced serum TAG.

158 Very cool low-mass white dwarfs must therefore have lost their thick hydrogen env

159 oides, semibrachytic, semidwarf, and slender dwarf mutant groups.

160 ons could unlock further yield gains in semi-dwarf mutants.

161 The narrow odd dwarf (nod) mutant displays defects at both the cellular

162 e pre-nova at minimum light with no trace of dwarf nova behaviour, implying that the mass-transfer ra

163 rs before the explosion, the system revealed dwarf nova outbursts indicative of a low mass-transfer r

164 d onto the white dwarf during quasi-periodic dwarf nova outbursts.

165 Another type of outburst is the dwarf nova: these occur in binaries that have stellar ma

166 a classical-nova event, the system exhibited dwarf-nova eruptions.

167 t lack firm post-eruption ages, and are also dwarf novae at present.

168 We conclude that many old novae become dwarf novae for part of the millennia between successive

169 discovery of ancient nova shells around the dwarf novae Z Camelopardalis and AT Cancri, but direct e

170 Cataclysmic variable stars-novae, dwarf novae, and nova-likes-are close binary systems con

171 same orbital period of novalike binaries and dwarf novae-which are identical but for their widely var

172 Here, we describe a rapid example of dwarfing of a large mammal - the feral cattle of Amsterd

173 The dwarfing of large mammals on islands has been observed b

174 e planetary population surrounding ultracool dwarfs, of which the TRAPPIST-1 planets are the first tr

175 hippopotami, deer, and other species became dwarfed on islands scattered all over the world, from th

176 peptide of 34 amino acids and that we named dwarf open reading frame (DWORF).

177 calized ignition on the surface of the white dwarf or as a consequence of rotational distortion.

178 se must either originate from near the white dwarf or be generated in situ at the M star through dire

179 vae resulted from the merger of binary white dwarfs or other compact stars such as helium stars.

180 ll either on a near-Chandrasekhar-mass white dwarf, or on a sub-Chandrasekhar-mass white dwarf mergin

181 phatase) of avp1-2 plants resulted in severe dwarf phenotype and abnormal leaf morphology.

182 lines showed reduced leaf number, leaf area, dwarf phenotype and delayed seed germination.

183 creen identifies T0 plants with the expected dwarf phenotype associated with knock-out of the target

184 atprx71-1 mutation partially suppresses the dwarf phenotype of qua2-1, suggesting that AtPRX71 contr

185 c expression of a hairpin construct led to a dwarf phenotype similar to that of dw/dw peaches.

186 Ectopic accumulation of IBH1 causes a severe dwarf phenotype, but the cell elongation suppression mec

187 ally normal while homozygotes demonstrated a dwarf phenotype.

188 gonst1 plants have a dwarfed phenotype and a constitutive hypersensitive resp

189 rom UABs of ACC-treated plants resulted in a dwarfed phenotype that mimicked the growth response in R

190 Knockdown of BoiCesA caused "dwarf" phenotype with smaller leaves and a loss of the c

191 In Chukotka, the total cover of alder and dwarf pine (Pinus) increased 6.1% within one ecotone and

192 Studies of the dwarf planet (1) Ceres using ground-based and orbiting t

193 The dwarf planet (1) Ceres, the largest object in the main a

194 the largest object in the asteroid belt, the dwarf planet (1) Ceres, which is thought to be different

195 The surface elemental composition of dwarf planet Ceres constrains its regolith ice content,

196 The surface of dwarf planet Ceres contains hydroxyl-rich materials.

197 The dwarf planet Ceres is known to host phyllosilicate miner

198 Dawn Framing Camera images, of a landform on dwarf planet Ceres that we argue represents a viscous cr

199 nic absorption feature at 3.4 micrometers on dwarf planet Ceres.

200 The dwarf planet is dominated by numerous craters, but other

201 tensor, resulting in a reorientation of the dwarf planet of around 60 degrees with respect to the ro

202 The 1,000-kilometre-diameter dwarf planet Sedna was discovered ten years ago and was

203 tive surface renewal may also occur on other dwarf planets in the Kuiper belt, which may help to expl

204 ts in great numbers: the average number of M-dwarf planets that are between 0.5 to 1.5 times the size

205 anets (radii less than 1.7 Earth radii), gas dwarf planets with rocky cores and hydrogen-helium envel

206 We also find that this low-mass white-dwarf precursor is a type of pulsating star not hitherto

207 ion radius) and then accretes onto the white dwarf, producing bursts powered by the release of gravit

208 y debris from the planetary systems of white-dwarf progenitors occasionally pollutes the atmospheres

209 omoting interventions, specifically the Ames dwarf Prop1 (df/df) mutation, calorie restriction and ra

210 At a distance of 1.295 parsecs, the red dwarf Proxima Centauri (alpha Centauri C, GL 551, HIP 70

211 ely 'Chinese Cavendish', 'Giant Cavendish', 'Dwarf Red', 'Grand Nain', 'Eilon', 'Gruesa', 'Silver', '

212 r spectrum of intermediate-temperature brown dwarfs resembles that of Neptune, indicating the presenc

213 Semi-dwarf rice varieties with low tiller formation but high

214 ar through direct interaction with the white dwarf's magnetosphere.

215 hough the pulsations are driven by the white dwarf's spin, they mainly originate from the cool star.

216 e we report a two-dimensional map of a brown dwarf's surface that allows identification of large-scal

217 cation of this is that a population of 'dark dwarfs' should orbit the Milky Way: halos devoid of star

218 Evergreen dwarf shrub biomass decreased (30%) following extreme wi

219 auses of growth variability of the evergreen dwarf shrub Cassiope tetragona between 1927 and 2012 in

220 Dwarf shrub dendrochronology may reveal climatological c

221 y influence C uptake and retention in Arctic dwarf shrub vegetation.

222 might promote an expansion of this evergreen dwarf shrub, mainly through densification of existing sh

223 Acutifolia and Pleurozium schreberi) and in dwarf shrub-P. schreberi vegetation in sub-Arctic Finlan

224 that of P. schreberi was 62-81% and that of dwarf shrub-P. schreberi vegetation was 58-74%.

225 ypically greater for exclosures dominated by dwarf shrubs (Calluna vulgaris) than by grasses (Molinia

226 Evergreen dwarf shrubs are disadvantaged in a future sub-Arctic wi

227 Our findings suggest that dwarf-shrubs and graminoids prime microbial decompositio

228 peatland carbon (up to 2100 years old) when dwarf-shrubs or graminoids are present, an effect not ob

229 The 'dwarf' smORFs are in general shorter (around 20 amino-ac

230 Channel Island fox (Urocyon littoralis) is a dwarfed species that inhabits six of California's Channe

231 of the satellite galaxies of Andromeda, the dwarf spheroidal Andromeda II, which has a mass of only

232 e of a plateau of europium abundance in some dwarf spheroidal galaxies has been suggested as evidence

233 s pattern has not been cleanly identified in dwarf spheroidals.

234 e close binary systems consisting of a white dwarf star (the primary) that is accreting matter from a

235 The M dwarf star Gliese 581 is believed to host four planets,

236 in the liquid-water, habitable zone of an M dwarf star is probably around 10.5 parsecs away.

237 SP-33b; the planet is itself as hot as a red dwarf star of type M (ref.

238 Earth-sized planets transiting an ultracool dwarf star only 12 parsecs away.

239 agration of an accreting carbon-oxygen white dwarf star or the explosion of an accreting, hybrid carb

240 much further out in the magnetosphere of the dwarf star that couple energy into the lower atmosphere.

241 stem of seven planets orbiting the ultracool dwarf star TRAPPIST-1 and find that panspermia is potent

242 transiting the recently discovered ultracool dwarf star TRAPPIST-1 are capable of retaining their atm

243 o the habitable zone of the nearby ultracool dwarf star TRAPPIST-1.

244 f the trajectory of an exoplanet around an M dwarf star, derived by mapping the spectrum of the stell

245 plosions, occurring on the surfaces of white dwarf stars accreting gas from companions in binary star

246 Isolated cool white dwarf stars more often have strong magnetic fields than

247 se from the thermonuclear explosion of white-dwarf stars that have cores of carbon and oxygen.

248 (SNe), the thermonuclear explosions of white-dwarf stars, vary systematically with their intrinsic co

249 M dwarf stars, which have masses less than 60 per cent tha

250 M-dwarf stars--hydrogen-burning stars that are smaller tha

251 detonation in accreting carbon-oxygen white-dwarf stars.

252 ant with reduced PtdIns(4,5)P2 levels showed dwarf stature and phenotypes suggesting defects in auxin

253 zmbri1-RNAi plants showed dwarf stature due to shortened internodes, with upper in

254 defects in growth and development, including dwarf stature, rolled leaves, and small seeds.

255 x) mutants, with collapsed xylem vessels and dwarfed stature, highlighted the importance of this cell

256 rolensing caused by a nearby star, the white dwarf Stein 2051 B.

257 The white dwarf stellar remnant and its Sun-like companion orbit o

258 The gravitational field of the outer white dwarf strongly accelerates the inner binary containing t

259 stars of extremely low mass as well as brown dwarfs (substellar objects not massive enough to sustain

260 Brown dwarfs--substellar bodies more massive than planets but

261 sks surrounding about four per cent of white dwarfs, suggests that rocky debris from the planetary sy

262 actic plane, is dominated by accreting white dwarf systems.

263 explosions of accreting carbon-oxygen white dwarfs that do not completely unbind the star, implying

264 action space of the continuous donation game dwarfs that of the classic prisoner's dilemma, players c

265 iability or other external forcings may have dwarfed the fairly modest ENSO response to precessional

266 which we relate to the microphysics of brown dwarfs through viscosity and electron collisions.

267 r models, we constrain the mass of the white dwarf to be ~63% of the mass of our Sun.

268 mass of Stein 2051 B-the sixth-nearest white dwarf to the Sun-as 0.675 +/- 0.051 solar masses.

269 sterdam Island, southern Indian Ocean, which dwarfed to about three quarters of its body size in slig

270 escope infrared monitoring campaign of brown dwarfs to constrain cloud cover variations over a total

271 s linked to the QTL may be used in selecting dwarf trees.

272 Barley yellow dwarf virus (BYDV) adversely affects the yield and quali

273 Barley yellow dwarf virus (BYDV) employs a cap-independent mechanism o

274 to transmit the RPV strain of Cereal yellow dwarf virus (CYDV-RPV).

275 lobal gene expression of Rice black-streaked dwarf virus (RBSDV)-infected rice plants with that of he

276 rns were evaluated for 229 isolates of Wheat dwarf virus (WDV), which are important cereal-infecting

277 s using a deconstructed version of the wheat dwarf virus (WDV).

278 tions among wheat (cv. Yitpi), Barley yellow dwarf virus and an important pest and virus vector, the

279 important in mRNA translation, barley yellow dwarf virus employs a novel mechanism utilizing the 3'-U

280 tabacum), replicons based on the bean yellow dwarf virus enhanced gene targeting frequencies one to t

281 Barley yellow dwarf virus mRNA, which lacks both cap and poly(A) tail,

282 Barley yellow dwarf virus RNA, lacking a 5' cap and a 3' poly(A) tail,

283 sativa with two virus species, barley yellow dwarf virus-PAV (BYDV-PAV) and cereal yellow dwarf virus

284 deaceus and the viral pathogen Barley yellow dwarf virus-PAV.

285 dwarf virus-PAV (BYDV-PAV) and cereal yellow dwarf virus-RPV (CYDV-RPV).

286 Yellow dwarf viruses cause the most economically important viru

287 ghtness and magnetic field of the cool white dwarf WD 1953-011 taken over about eight years, and the

288 Here we report observations of a white dwarf--WD 1145+017--being transited by at least one, and

289 che environments that benefit the endangered dwarf wedgemussel (Alasmidonta heterodon).

290 seeps were identified at all locations where dwarf wedgemussels still can be found.

291 They reflect the spin of a magnetic white dwarf, which we find to be slowing down on a 10(7)-year

292 ong magnetic fields than young, hotter white dwarfs, which has been a puzzle because magnetic fields

293 er the entire surface in cool magnetic white dwarfs, which inhibits their cooling evolution relative

294 dly along the poles as a wind from the white dwarf, while denser material drifted out along the equat

295 ernovae deriving from the explosion of white dwarfs with mass above the Chandrasekhar limit is in agr

296 In addition, some white dwarfs with strong fields vary in brightness as they rot

297 Mutant up plants grown in vitro were dwarf, with abundant axillary shoot growth, greater tube

298 e Carina, the eighth most luminous Milky Way dwarf, would be expected to inhabit a significantly more

299 r confirmed by sequencing the Dw2 alleles in Dwarf Yellow Milo and Double Dwarf Yellow Milo, the prog

300 Dw2 alleles in Dwarf Yellow Milo and Double Dwarf Yellow Milo, the progenitor genotypes where the re

301 the connections between accretion onto white dwarfs, young stellar objects and neutron stars, for whi