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1 cloud is hot, dense, quiescent and extremely dusty.
2 than the Viking landing sites but comparably dusty.
3 active galactic nuclei, the orientation of a dusty accretion torus around the central black hole domi
4  z 5.8 indeed suggest that these systems are dusty and may be caught during an initial quenching phas
5  collected during two spring seasons on both dusty and nondusty days.
6 .4 ml, and 0.1 % per year of employment in a dusty area, respectively, whereas the association betwee
7 king status, pack-years, and years worked in dusty areas were examined using stepwise multiple linear
8                                          The dusty atmosphere of Mars undergoes aeolian processes, ra
9 lts are consistent with the warm, moderately dusty atmosphere seen by VL-1.
10 higher particle precipitation, or under less dusty atmospheric conditions, aurorae will be visible to
11  low-density, highly porous (72-74 per cent) dusty body, similar to that of comet 9P/Tempel 1.
12 n and excess infrared emission-signatures of dusty circumstellar disks(12), stellar activity(13) and
13                  Stars form with gaseous and dusty circumstellar envelopes, which rapidly settle into
14                    We report observations of dusty clouds in Saturn's rings, which we interpret as re
15 craft exhaust plumes and lunar soil produces dusty clouds with high-speed particle ejection.
16  suggested evolutionary effects(2) and added dusty clumps and polar winds(3) but left the basic pictu
17                                         This dusty combination of smog and ethane, forming deposits s
18 nt to the cross-sectional area of the ring's dusty component.
19 observed variations in both the volatile and dusty components of comets, while also providing a natur
20 by 0.2-0.4 from clean to polluted, smoky, or dusty conditions.
21  applications, medical imaging, and foggy or dusty conditions.
22         Over the northern Great Plains, less dusty days are expected in spring due to increased preci
23 olar radiation intensities and the number of dusty days parameters indicate that the fuzzy_DS method
24  a carbon monoxide gas ring co-orbiting with dusty debris around HD 172555 between about six and nine
25                               The star has a dusty debris disk, and the star's spectrum shows promine
26 s fact, together with the existence of warm, dusty debris disks surrounding about four per cent of wh
27 retical studies show that the structure of a dusty disk can be modified by the gravitational influenc
28 l evidence, such as the detection of compact dusty disks around massive young stellar objects, is nee
29 5 per cent of nearby stars are surrounded by dusty disks that must be collisionally replenished by as
30  daily, over 25% of which were significantly dusty ("dust devils").
31 ve of a small object with a cometary tail of dusty effluent material.
32  gone from hosting substantial quantities of dusty ejecta, in a region analogous to where the rocky p
33 GB) stars eject material that forms extended dusty envelopes(1).
34 el environmental sensors and Jezero crater's dusty environment remedy this.
35                               Discovery of a dusty environment, a natural satellite, or unexpected as
36 hood dustiness, ranging from 5% in the least dusty environments to 12% in the dustiest (p for trend =
37 udies showing increased risk associated with dusty environments.
38                                              Dusty, evolved galaxies are thus present among the faint
39                               A less or more dusty future depends on temperature variations in the No
40 es to centuries can result in a less or more dusty future.
41         Such a high abundance of massive and dusty galaxies in the early Universe challenges our unde
42 e growth of massive black holes and luminous dusty galaxies.
43 1(01)) line due to starburst activity in the dusty galaxy HFLS3 results in a cooling to below the red
44 oles that reveals that radiative feedback on dusty gas is the main physical mechanism that regulates
45 insic permeability is performed based on the dusty gas model (DGM) by considering the contribution of
46 mic history, black-hole growth occurs in the dusty, gas-rich centres of active galaxies.
47 brightest star-forming regions, while in the dusty halo the field lines form a giant magnetic bubble
48 positive response of marine N(2) fixation to dusty ice age conditions, first proposed twenty years ag
49  caused by constructive interference between dusty ice layers that are more closely spaced than the r
50 moking, low level of education, working in a dusty job for more than 10 years, previous tuberculosis,
51                                          The dusty jovian ring system must be replenished continuousl
52    The measured redshift (z) distribution of dusty, massive starbursts has long been suspected to be
53 d as variations in the surface area of warm, dusty material ejected by planetary-scale collisions and
54 ic measurement scheme, inspired by Newton's 'dusty mirror' experiment, to monitor the X-ray-induced e
55 terstellar medium (ISM) through a processed, dusty, molecular wind.
56 hly likely to be underestimated, even in the dusty North Atlantic.
57 gion is affected by the Harmattan, a dry and dusty northeasterly trade wind blowing from the Sahara i
58 wristbands deployed over a single shift in a dusty occupational setting can be useful for indicating
59                            Here we show that dusty olivine-bearing chondrules from the Semarkona mete
60 ry descriptors mushroom, cellar-like, musty, dusty or metallic.
61  We show that this is due to the presence of dusty plasma in the near-equatorial ionosphere.
62                                              Dusty plasma is a mixture of ions, electrons, and macros
63 ntuition to infer force laws in a laboratory dusty plasma.
64  hidden, and may be in environments that are dusty, rainy, dark and/or in deep forest.
65  that resulted in complete vaporization of a dusty region of the solar nebula (dust/gas ratio of abou
66 ecasting and regional climate predictions in dusty regions.
67 's G ring, which is red, a typical color for dusty rings.
68  the emission arises from gas inside a cold, dusty, rotating disk with a rotational velocity of about
69 how that accounting for a vegetated and less dusty Sahara during the mid-Holocene relative to preindu
70 were more frequently isolated during the dry dusty season of the year.
71 nterpreted as finegrained ocean sediments or dusty snow.
72                                          The dusty soil on the Moon, called lunar regolith, is known
73 the statistical and individual properties of dusty star-forming galaxies.
74 ared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star f
75 r-Eddington black-hole accretion disk at the dusty starburst core.
76 ie at z > 4, indicating that the fraction of dusty starburst galaxies at high redshifts is greater th
77 volutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant
78 red a population of luminous, high-redshift, dusty starburst galaxies.
79 in near-infrared color-magnitude diagrams of dusty substellar atmospheres.
80 ule heating on convective stretching flow of dusty tangent hyperbolic fluid over a sheet in 3D.
81 inflow has been measured at the scale of the dusty torus that surrounds the central accretion disk(5)
82 aunching radius comparable to the scale of a dusty torus, indicating that the coupling between dust a
83 10 centimeters but appear to be covered by a dusty veneer in places, which may obscure thinner layers
84 ir sticky feet from fouling while running on dusty walls and ceilings.
85         Recent Mars exploration has revealed dusty, water-ice-rich mantling deposits that are layered
86 onments, respectively, likely because of the dusty work environment and greater movement of e-waste w