ライフサイエンスコーパス: dusty

1 than the Viking landing sites but comparably dusty.

2 cloud is hot, dense, quiescent and extremely dusty.

3 collected during two spring seasons on both dusty and nondusty days.

4 .4 ml, and 0.1 % per year of employment in a dusty area, respectively, whereas the association betwee

5 king status, pack-years, and years worked in dusty areas were examined using stepwise multiple linear

6 lts are consistent with the warm, moderately dusty atmosphere seen by VL-1.

7 low-density, highly porous (72-74 per cent) dusty body, similar to that of comet 9P/Tempel 1.

8 Stars form with gaseous and dusty circumstellar envelopes, which rapidly settle into

9 We report observations of dusty clouds in Saturn's rings, which we interpret as re

10 This dusty combination of smog and ethane, forming deposits s

11 nt to the cross-sectional area of the ring's dusty component.

12 observed variations in both the volatile and dusty components of comets, while also providing a natur

13 by 0.2-0.4 from clean to polluted, smoky, or dusty conditions.

14 Over the northern Great Plains, less dusty days are expected in spring due to increased preci

15 The star has a dusty debris disk, and the star's spectrum shows promine

16 s fact, together with the existence of warm, dusty debris disks surrounding about four per cent of wh

17 retical studies show that the structure of a dusty disk can be modified by the gravitational influenc

18 l evidence, such as the detection of compact dusty disks around massive young stellar objects, is nee

19 5 per cent of nearby stars are surrounded by dusty disks that must be collisionally replenished by as

20 ve of a small object with a cometary tail of dusty effluent material.

21 gone from hosting substantial quantities of dusty ejecta, in a region analogous to where the rocky p

22 hood dustiness, ranging from 5% in the least dusty environments to 12% in the dustiest (p for trend =

23 udies showing increased risk associated with dusty environments.

24 Dusty, evolved galaxies are thus present among the faint

25 A less or more dusty future depends on temperature variations in the No

26 es to centuries can result in a less or more dusty future.

27 e growth of massive black holes and luminous dusty galaxies.

28 oles that reveals that radiative feedback on dusty gas is the main physical mechanism that regulates

29 insic permeability is performed based on the dusty gas model (DGM) by considering the contribution of

30 mic history, black-hole growth occurs in the dusty, gas-rich centres of active galaxies.

31 brightest star-forming regions, while in the dusty halo the field lines form a giant magnetic bubble

32 The dusty jovian ring system must be replenished continuousl

33 The measured redshift (z) distribution of dusty, massive starbursts has long been suspected to be

34 ic measurement scheme, inspired by Newton's 'dusty mirror' experiment, to monitor the X-ray-induced e

35 terstellar medium (ISM) through a processed, dusty, molecular wind.

36 gion is affected by the Harmattan, a dry and dusty northeasterly trade wind blowing from the Sahara i

37 Here we show that dusty olivine-bearing chondrules from the Semarkona mete

38 hidden, and may be in environments that are dusty, rainy, dark and/or in deep forest.

39 that resulted in complete vaporization of a dusty region of the solar nebula (dust/gas ratio of abou

40 ecasting and regional climate predictions in dusty regions.

41 's G ring, which is red, a typical color for dusty rings.

42 how that accounting for a vegetated and less dusty Sahara during the mid-Holocene relative to preindu

43 nterpreted as finegrained ocean sediments or dusty snow.

44 the statistical and individual properties of dusty star-forming galaxies.

45 ared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star f

46 ie at z > 4, indicating that the fraction of dusty starburst galaxies at high redshifts is greater th

47 volutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant

48 red a population of luminous, high-redshift, dusty starburst galaxies.

49 10 centimeters but appear to be covered by a dusty veneer in places, which may obscure thinner layers

50 ir sticky feet from fouling while running on dusty walls and ceilings.

51 Recent Mars exploration has revealed dusty, water-ice-rich mantling deposits that are layered