ライフサイエンスコーパス: milky

1 om 4000 to 6000 mg/dl, and the plasma turned milky.

2 ries was that of ripe fruit, followed by the milky and chemical series.

3 y nucleate in the whole drop, leading to its milky color that typifies the so-called "Ouzo effect." O

4 The presence of a milky, creamy appearing ascitic fluid with triglyceride

5 h-quality natural rubber in their latex, the milky cytoplasm of specialized cells known as laticifers

6 investigate 20 to 200 nm sized inclusions in milky diamonds from Rio Soriso, Juina area, Brazil.

7 ng beetle, Thermonectus marmoratus, ejects a milky fluid from its prothoracic defensive glands when d

8 Gpihbp1 knockout mice on a chow diet have milky plasma and plasma triglyceride levels of more than

9 (basalt, granite, hematite, magnetite, mica, milky quartz, and clear quartz) to quantify the capillar

10 lue-white veil, pink color, black color, and milky red/pink areas.

11 f scientific observations, an explanation of milky seas has remained elusive.

12 ny light-emitting organism, these so-called "milky seas" are hypothesized to be manifestations of unu

13 se genetic background does not alter omental milky spot number and size, nor does it affect ovarian c

14 Similarly, medium conditioned by milky spot-containing adipose tissue caused 75% more cel

15 ell migration than did medium conditioned by milky spot-deficient adipose.

16 um also contains lymphoid aggregates, called milky spots (MSs), that contribute to peritoneal immunit

17 e present study shows the novel finding that milky spots and adipocytes play distinct and complementa

18 dings support a two-step model in which both milky spots and adipose have specific roles in colonizat

19 ally associated with lymph nodes and omental milky spots have site-specific properties that equip the

20 Unlike conventional lymphoid organs, milky spots in the omentum developed in the absence of l

21 These results indicate that the milky spots of the omentum function as unique secondary

22 Omental milky spots readily concentrate intra-abdominal E. coli

23 Although the lymphoid architecture of milky spots was disrupted in lymphotoxin-deficient mice,

24 This tissue is unusual for its milky spots, comprised of immune cells, stromal cells, a

25 omental and splenoportal fat, which contain milky spots, rather than in peritoneal fat depots.

26 PWC5 variety of purple waxy corn at the milky stage had the highest values for all parameters, a

27 TPC and TAC were highest at the milky stage, whereas TFC and AA were highest at the silk

28 I also estimate the age of the Milky Way (14.5(+2.8)(-2.2)Gyr in a way that is independ

29 ources further than the sun (both within the Milky Way and beyond) are expected to produce a flux of

30 00 K) foreground synchrotron emission in the Milky Way and extragalactic continuum sources.

31 nding of the globular cluster systems of the Milky Way and other galaxies point to a complex picture

32 ews recent studies of collisions between the Milky Way and smaller satellite galaxies.

33 expected for this line of sight through the Milky Way and the intergalactic medium, indicating magne

34 arm as it passes through the far side of the Milky Way and to validate a kinematic method for determi

35 of the Local Group of galaxies to which the Milky Way belongs are shedding light on some of the proc

36 The Milky Way bulge underwent a rapid chemical enrichment du

37 vations of extremely metal-poor stars in the Milky Way bulge, including one star with an iron abundan

38 asonably well constrained in the disk of the Milky Way but we have very little direct information on

39 many more low-mass stars than the IMF in the Milky Way disk, and was probably slightly steeper than t

40 ace density of neutral hydrogen in the outer Milky Way disk, demonstrating that the Galaxy is a non-a

41 ost of the dark matter subhalos orbiting the Milky Way do not host visible galaxies.

42 But the Milky Way does not seem to have suffered any major colli

43 Otherwise Carina, the eighth most luminous Milky Way dwarf, would be expected to inhabit a signific

44 al-poor globular clusters in the halo of the Milky Way formed in dwarf galaxies, as is commonly belie

45 ation may indicate that galaxies such as the Milky Way gain much of their mass by accretion rather th

46 rbiting a few relatively normal stars in our Milky Way Galaxy and also at the centers of some galaxie

47 The Milky Way galaxy contains a large, spherical component w

48 ner tens of light-years at the center of the Milky Way Galaxy contains five principal components that

49 The Milky Way galaxy has several components, such as the bul

50 stars in the central few light years of our Milky Way Galaxy indicate the presence of a dark object

51 rvations of stellar globular clusters in the Milky Way Galaxy, combined with revised ranges of parame

52 During the lifetime of our Milky Way galaxy, there have been something like 100 mil

53 kelvin interstellar medium component in the Milky Way Galaxy.

54 mmon in much older supernova remnants in the Milky Way Galaxy.

55 ation events thought to originate beyond the Milky Way galaxy.

56 ce of two flat-spectrum radio sources in the Milky Way globular cluster M22, and we argue that these

57 other star ('black-hole/X-ray binaries') in Milky Way globular clusters, even though many neutron-st

58 e associated constraints on the shape of the Milky Way gravitational potential, treating the Sgr impa

59 dies of trends in chemical abundances in old Milky Way halo stars suggested that these elements are p

60 ld in the central few hundred parsecs of the Milky Way has a dipolar geometry and is substantially st

61 The Milky Way has at least twenty-three known satellite gala

62 e velocities of stars near the centre of the Milky Way have provided the strongest evidence for the p

63 Like many galaxies of its size, the Milky Way is a disk with prominent spiral arms rooted in

64 Most of the matter in the Milky Way is invisible to astronomers.

65 Little is known about the portion of the Milky Way lying beyond the Galactic center at distances

66 rate integrated over the entire disk of the Milky Way of approximately 1 solar mass per year can sol

67 uter haloes of massive galaxies, such as the Milky Way or Andromeda.

68 dium pervading an extended corona around the Milky Way or the Local Group.

69 result demonstrates that the faintest of the Milky Way satellites are the most dark-matter-dominated

70 t been found in the chemical compositions of Milky Way stars.

71 Models of the chemical evolution of the Milky Way suggest that the observed abundances of elemen

72 und star clusters (globular clusters) in the Milky Way suggests that efficiencies were higher when th

73 we report simulations of the response of the Milky Way to the infall of the Sagittarius dwarf galaxy

74 lar gas is also low, about 3 per cent of the Milky Way value.

75 city is approximately one-thousand times the Milky Way value.

76 drogen content of luminous galaxies like the Milky Way within 100 million years.

77 dark matter halos and the properties of the Milky Way's dwarf galaxy satellites.

78 nces have been seen in selected stars in the Milky Way's halo and in two quasar absorption systems at

79 Our results show that the Milky Way's morphology is not purely secular in origin a

80 3.6(-2.3)(+3.8) x 10(8) Msun for one of the Milky Way's satellites: Carina.

81 urrent cosmological models indicate that the Milky Way's stellar halo was assembled from many smaller

82 r for star formation in galaxies such as our Milky Way) remains unclear.

83 ts at the centres of galaxies similar to the Milky Way).

84 at a rate more than 2,000 times that of the Milky Way, a rate among the highest observed at any epoc

85 formed white dwarf stars in the halo of the Milky Way, and a separate analysis of archival data in t

86 y four such maximal sources are known in the Milky Way, and the absorption of soft X-rays in the inte

87 star indicate that it is in the halo of the Milky Way, and the density of such objects implied by th

88 In the Milky Way, high-mass stars form in the dense cores of in

89 Observations of supernova remnants in the Milky Way, however, have hitherto revealed only 10(-7)-1

90 on of luminous and nonluminous matter in the Milky Way, in galaxies, and in galaxy clusters.

91 ared and X-ray emission at the centre of the Milky Way, is the closest example of this phenomenon, wi

92 supermassive black hole at the center of the Milky Way, known as Sagittarius A* (Sgr A*), may have af

93 t active and heavily processed region of the Milky Way, so it can be used as a stringent test for the

94 Unlike spiral galaxies such as the Milky Way, the majority of the stars in massive elliptic

95 of low-metallicity stars in the halo of the Milky Way, to determine the U/Th production ratio very p

96 ith those measured from sources of CH in the Milky Way, we test the hypothesis that fundamental const

97 ormation predict many more subhalos around a Milky Way-like galaxy than the number of observed satell

98 II, a high-resolution N-body simulation of a Milky Way-sized galaxy, to investigate the phase-space s

99 be a nearby low-mass star in the disk of the Milky Way.

100 much of the 'dark matter' in the halo of the Milky Way.

101 e cloud that is falling into the disk of the Milky Way.

102 alaxies and in the extreme outer disk of the Milky Way.

103 es and column densities for CO clouds in the Milky Way.

104 s 50 per cent, tenfold that of clouds in the Milky Way.

105 n found in the outer regions ('halo') of the Milky Way.

106 ith a dust-to-gas ratio close to that of the Milky Way.

107 )-10(10 )Msun at the time they fell into the Milky Way.

108 factor of 100 greater than that seen in the Milky Way.

109 eir routes to the band of stars known as the Milky Way.

110 ittarius galaxy, which is a satellite of the Milky Way.

111 ar to that of the Sagittarius dwarf near the Milky Way.

112 al galaxies may not have the same IMF as the Milky Way.

113 sive black hole, SgrA*, at the centre of the Milky Way.

114 one of the most massive binary stars in the Milky Way.

115 th a spheroidal component, including our own Milky Way.

116 titude arcs observed in the same area of the Milky Way.

117 at are similar to population II stars in the Milky Way.

118 relatively rare in galaxies such as our own Milky Way.

119 probe the chemical enrichment history of the Milky Way.

120 greater than 30, in the early history of the Milky Way.

121 ss was temporarily the brightest star in the Milky Way.

122 population of 'dark dwarfs' should orbit the Milky Way: halos devoid of stars and yet more massive th