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 ccretion rate that we observe onto the white dwarf.

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

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

5 onuclear runaway on the surface of the white dwarf.

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

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

8 million, which is unusually quiet for a red dwarf.

9 o planet has so far been detected at a white dwarf.

10 y evolve into red giants and then into white dwarfs.

11 e giant planets in close orbits around white dwarfs.

12 isk instabilities drop matter onto the white dwarfs.

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

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

15 nse plasma related to the viscosity of brown dwarfs.

16 estructive explosions of carbon-oxygen white dwarfs.

17 objects such as brown-dwarf cores and white dwarfs.

18 for smaller transiting planets around white dwarfs.

19 e been detected in close orbits around white dwarfs.

20 enriched outer layers, leaving behind white dwarfs.

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

22 ID1c silencing corresponded to the degree of dwarfing.

23 Conversely, LOH2 overexpression resulted in dwarfing.

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

25 ne the age of stellar populations from white dwarfs(10).

26 an intermediate-mass black hole and a white dwarf(13).

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

28 thod to measure the wind speeds on the brown dwarf 2MASS J10475385+2124234.

29 Close to the upper mass limit of a white dwarf(3) (1.4 solar masses), rapid accretion of hydrogen

30 s phase and remain in orbit around the white dwarf(3,4).

31 hotospheric trace metals found in many white dwarfs(3) arise from the accretion of tidally disrupted

32 red giants(3), high-mass stars(4) and white dwarfs(5).

33 ll other known planetary debris around white dwarfs(7), but resembles predictions for the makeup of d

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

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

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

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

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

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

40 The gid1 triple mutant was extremely dwarf and fully insensitive to GA.

41 tify two phyB mutant alleles that revert the dwarf and high salicylic acid phenotypes of the high MEc

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

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

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

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

46 the disease symptoms caused by RGSV, such as dwarfing and excess tillering, in transgenic rice plants

47 levels and whole-plant phenotypes, including dwarfing and spontaneous cell death lesions.

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

49 ions that are used in the modelling of white dwarfs and inertial confinement fusion experiments(7,8),

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

51 iple, this technique can be applied to brown dwarfs and/or directly imaged exoplanets if periods can

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

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

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

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

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

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

58 gh-energy-density states that exist in white dwarfs are extremely difficult to reach and to measure i

59 Brown dwarfs are massive analogs of extrasolar giant planets a

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

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

62 White dwarfs are stellar embers depleted of nuclear energy sou

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

64 ch only one(5) is eclipsing-the double-white-dwarf binary SDSS J065133.338+284423.37, which has an or

65 t the discovery of an eclipsing double-white-dwarf binary system, ZTF J153932.16+502738.8, with an or

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

67 ecord tightly constrains the colonization of dwarf birch (Betula, a thermophilous shrub) to 5.9 +/- 0

68 demonstrated in Triticum aestivum 'Apogee' (dwarf bread wheat) and resulted in an 18% increase in gr

69 thway genes can be an effective approach for dwarfing breeding of turf grasses.

70 previously puzzling behaviors seen in brown dwarf brightness variations.

71 d to differing developmental modes (Clade V: dwarf brooder vs. Clade I: giant broadcaster).

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

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

74 ind their way into tight orbits around white dwarfs, but it is unclear whether these planets can surv

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

76 these locations, they were likely small and dwarfed by contemporary P sources.

77 ombination events in cis, an outcome that is dwarfed by pervasive accompanying undesired editing even

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

79 reaks occurred at the same time as, and were dwarfed by, seasonal epidemics of influenza types A and

80 bsequent accretion of planetesimals by white dwarfs can reveal the elemental abundances of rocky bodi

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

82 d modelled the periodic dimming of the white dwarf caused by the planet candidate passing in front of

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

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

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

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

87 t-order phase transition occurs during white-dwarf cooling, leading to the crystallization of the non

88 iors and astrophysical objects such as brown-dwarf cores and white dwarfs.

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

90 ase of latent heat as the cores of the white dwarfs crystallize.

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

92 ere distinct from those associated with semi-dwarf cultivars, with higher differential abundance of A

93 ities in the tall cultivars relative to semi-dwarf cultivars.

94 ia, Planctomycetes and Acidobacteria in semi-dwarf cultivars.

95 These figures dwarf current, typically inadequate spending on conservi

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

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

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

99 ich has a lesion in the BR biosynthetic gene DWARF (DWF), and in the bzr1 mutant, which is deficient

100 low N include CONSTITUTIVE PHOTOMORPHOGENIC DWARF, DWF4, and BRASSINOSTEROID-6-OXIDASE 2 Phenotypic

101 Mutation of OsPIP5K1 compounds the dwarf dwt1 phenotype but abolishes the main shoot domina

102 erize the Arabidopsis (Arabidopsis thaliana) dwarf eceriferum11 (cer11) mutant and we show that it ex

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

104 lluminate the equation of state of the white dwarf envelope (the region surrounding the stellar core

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

106 tant had morphological changes that included dwarfing, excessive shoot branching and adventitious roo

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

108 100-1,000 km above the surface of the white dwarf, far too small to be resolved with current telesco

109 lated, supporting a previous conjecture that dwarf Flying Dragon originated as a mutant of a non-dwar

110 , and calcium in the atmosphere of the white dwarf Gaia DR2 4353607450860305024, which we ascribe to

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

112 cent developments-including the discovery of dwarf galaxies associated with the Magellanic group(14-1

113 ge galaxies grow through the accumulation of dwarf galaxies(1,2).

114 gned with the rotation axis for the plane of dwarf galaxies(14) that encircles M31.

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

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

117 ized to the largest star-forming region of a dwarf galaxy at a cosmological redshift of 0.19 (refs.

118 ized to the largest star-forming region of a dwarf galaxy at a cosmological redshift of 0.19 (refs. (

119 ations of stars rich in such elements in the dwarf galaxy Reticulum II(14), as well as the Galactic c

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

121 as localized to a low-metallicity, irregular dwarf galaxy, and the apparently non-repeating sources w

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

123 We provide an example using the homeologous dwarfing genes of allohexaploid wheat, Rht-1, and search

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

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

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

127 e subunits and enhances our understanding of dwarfing in phenylpropanoid pathway mutants.

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

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

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

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

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 haracterized the gut microbiomes of stranded dwarf (Kogia sima) and pygmy (K. breviceps) sperm whales

135 nerate a reference genome for the fat-tailed dwarf lemur, Cheirogaleus medius, and use this resource

136 Such is the case with Madagascar's dwarf lemurs (genus Cheirogaleus), the only obligate hib

137 e-wide estimates of genetic diversity within dwarf lemurs.

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

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

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

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 These white dwarfs may also later merge and synthesize elements as w

144 to facilitate a better understanding of the dwarfing mechanism in grasses at physiological and trans

145 l and transcriptional analyses to reveal the dwarfing mechanism in the mutant.

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

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 itro, and is also evident in Dnmt3a(W326R/+) dwarf mice.

151 nvestigated the influence of western hemlock dwarf mistletoe (Arceuthobium tsugense) on large (>=45.7

152 ese results imply that parasitic plants like dwarf mistletoe can amplify the impact of climatic stres

153 d that warmer and drier conditions amplified dwarf mistletoe effects on T. heterophylla tree growth a

154 The dwarf mistletoe rating (DMR), a measure of infection int

155 ting stars provides stringent tests of white dwarf models and a detailed picture of the outcome of th

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

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

158 nik1 plants exhibit dwarfed morphology, enhanced disease resistance to bacte

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

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

161 A transcriptomic comparison between the dwarf mutant and the WT leaves revealed 360 differential

162 In this study, we describe a dwarf mutant of Z. matrella induced from the (60)Co-gamm

163 Phenotypically, the dwarf mutant showed shorter stems, wider leaves, lower c

164 we found that the phenotypic changes of the dwarf mutant were associated with the physiological resp

165 on to the phenotypic changes observed in the dwarf mutant.

166 wild-type (Col-0) or rescue of GA-deficient dwarf mutants.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

183 an transmembrane proteins endoregulin (ELN), dwarf open reading frame (DWORF), myoregulin (MLN), and

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

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

186 Other cases of white dwarfs with close brown dwarf or stellar companions are explained as the consequ

187 red with other white dwarfs with close brown dwarf or stellar companions) and low mass of the planet

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

189 enveloped in a H(2)-He gaseous envelope (gas dwarfs) or contain a significant amount of multicomponen

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

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

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

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

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

195 ally normal while homozygotes demonstrated a dwarf phenotype.

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

197 e C(3) model system Brachypodium led to mild dwarf phenotypes, increased lignin (~7% to 13%) and S-li

198 tmospheres, where the understanding of white dwarf physics is sensitive to the equation of state and

199 Dawn mapping of dwarf planet (1) Ceres has identified similar deposits w

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

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

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

203 The dwarf planet Ceres is known to host phyllosilicate miner

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

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

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

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

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

209 ht wheat cultivars ranging from tall to semi-dwarf plants grown under field conditions.

210 results suggest that the development of semi-dwarf plants might have affected the ability of plants t

211 n in Arabidopsis plants resulted in severely dwarfed plants that could be rescued by the exogenous ap

212 e elemental abundances observed in six white dwarfs polluted by the accretion of rocky bodies to dete

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

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

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

216 Certain classes of white dwarfs pulsate(4,5), leading to observable brightness va

217 White dwarfs represent the final state of evolution for most s

218 cattering of planetesimals towards the white dwarf requires the presence of more massive bodies(6), y

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

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

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

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

223 nating from the debris disc around the white dwarf SDSS J122859.93+104032.9.

224 Some white dwarfs show evidence for rocky material floating in thei

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

226 Dwarf shrub dendrochronology may reveal climatological c

227 ) ) was carried out in widespread sub-Arctic dwarf shrub heathland, incorporating both mortality and

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

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

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

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

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

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

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

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

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

237 detection(1) of a dust disk around the white dwarf star G29-38 and transits from debris orbiting the

238 per-Earth exoplanets orbiting the nearby red dwarf star GJ 887.

239 The accretion of hydrogen onto a white dwarf star ignites a classical nova eruption(1,2)-a ther

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

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

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

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

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

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

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

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

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

249 Many white dwarf stars show signs of having accreted smaller bodies

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

251 forming the structure and evolution of white dwarf stars(9).

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

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

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

255 vae (SNIa)-thermonuclear explosions of white dwarf stars-is an open question in astrophysics.

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

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

258 rage stalk diameter and mechanical strength, dwarf stature, senescence at leaf tips, and semisterilit

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

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

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

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

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

264 pacers sequenced from a single sampling site dwarf the diversity of spacers from all available Sulfol

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

266 mately 25% of cis heritability across genes (dwarfing the contributions of other frequencies).

267 operations of America's state park systems, dwarfing the influence of climate change, which is signi

268 st important cardiovascular risk factor that dwarfs the impact of traditional risk factors.

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

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

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

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

273 rops, similar to the "green revolution" semi-dwarf trait in cereals, is a key plant architecture trai

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

275 lying Dragon originated as a mutant of a non-dwarfing type.

276 Dwarf varieties of Z. matrella are attractive to growers

277 Forest dwarfing via the gradual removal of taller trees by cycl

278 Barley Yellow Dwarf Virus (BYDV) is a positive strand RNA virus that l

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

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

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

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

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

284 re we show that a plant virus, barley yellow dwarf virus, increases the surface temperature of infect

285 and transits from debris orbiting the white dwarf WD 1145+017 (ref.

286 giant planet candidate transiting the white dwarf WD 1856+534 (TIC 267574918) every 1.4 days.

287 ning PSR J1141-6545 includes a massive white dwarf (WD) companion that formed before the gravitationa

288 roscopy of a hot (about 27,750 kelvin) white dwarf, WD J091405.30+191412.25, that is accreting from a

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

290 The development of dwarf wheat cultivars combined with high levels of agroc

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

292 A giant planet orbiting a hot white dwarf with a semi-major axis of around 15 solar radii wi

293 Other cases of white dwarfs with close brown dwarf or stellar companions are

294 ng orbital period (compared with other white dwarfs with close brown dwarf or stellar companions) and

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

296 up in the cooling sequence of evolving white dwarfs within 100 parsecs of the Sun, determined using p

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

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

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

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