Results 111 to 120 of about 5,588,447 (203)
A Detection of Circumgalactic Dust at Megaparsec Scales with Maximum Likelihood Estimation
The Astrophysical JournalOne of the more surprising astrophysical discoveries of the past decade has been the presence of enormous quantities of dust at megaparsec distances from galaxies, which has important implications for galaxy evolution, the circumgalactic and ...
Jacqueline E. McCleary +3 more
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88th Annual Meeting of the Meteoritical Society 2026: Contents
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S2-S47, August 2026.
wiley +1 more source
Inhomogeneous Dust Biases Photometric Redshifts and Stellar Masses for LSST
The Astrophysical Journal LettersSpectral energy distribution (SED) modeling is one of the main methods to estimate galaxy properties, such as photometric redshifts, z , and stellar masses, M _* , for extragalactic imaging surveys.
ChangHoon Hahn, Peter Melchior
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88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source
The Astrophysical JournalThe formation and survival of complex organic molecules (COMs) in cold interstellar environments depends on their interactions with icy dust grain surfaces.
Aneesa Ahmad +4 more
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, 1989 Coagulation is an important mechanism in the growth of interstellar and interplanetary dust particles. The microphysics of the coagulation process was theoretically analyzed as a function of the physical properties of the coagulating grains, i.e., their ...
Hollenbach, David +2 more
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Photocleavage of Aliphatic C–C Bonds in the Interstellar Medium
The Astrophysical JournalUltraviolet (UV) processing in the interstellar medium (ISM) induces the dehydrogenation of hydrocarbons. Aliphatics, including alkanes, are present in different interstellar environments, being prevalently formed in evolved stars; thus, the ...
Guillermo Tajuelo-Castilla +8 more
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The Astrophysical JournalWith the advent of JWST ice observations, dedicated studies on the formation reactions of detected molecules are becoming increasingly important. One of the most interesting molecules in interstellar ice is CO _2 .
Atsuki Ishibashi +5 more
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Interstellar and cometary dust [PDF]
, 1989 Aspects of interstellar dust which are known from direct observation will be discussed. Some specific difficulties that various theories have in explaining the observations will be presented.
Mathis, John S.
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Sensitivity of Polarization to Grain Shape. II. Aggregates
The Astrophysical JournalA previous study (Paper I) investigated the polarization properties of a variety of simple convex grain shapes, some of which were found to be consistent with the observed polarization properties of interstellar dust from far-ultraviolet to far-infrared.
B. T. Draine
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