Results 231 to 240 of about 437,551 (293)

X-ray absorption spectroscopy of FeH⁺ to aid its identification in astrochemical environments.

Chem Commun (Camb)
Jin S, Flach M, Ebenbichler A, Cunningham EM, Zamudio-Bayer V, Hirsch K, van der Linde C, Przybilla N, Ončák M, Lau JT, Beyer MK.   +10 more
europepmc   +1 more source

Hydrogen ejection from hydrocarbons: Characterization and relevance in soot formation and interstellar chemistry. [PDF]

Proc Natl Acad Sci U S A
Hendrix J, Hait D, Michelsen HA, Head-Gordon M.   +3 more
europepmc   +1 more source

The Origins & Reservoirs of Exocomets. [PDF]

Space Sci Rev
Bannister M, Pfalzner S, Pearce T, Mustill AJ, Klahr H, Nomura H, Ohashi N, Kokotanekova R, Marino S, Bodewits D, Marschall R, Seligman DZ, Jones GH, Veras D.   +13 more
europepmc   +1 more source

Formation of S-Bearing Complex Organic Molecules in Interstellar Clouds via Ice Reactions with C₂H₂, HS, and Atomic H. [PDF]

ACS Earth Space Chem
Santos JC, Enrique-Romero J, Lamberts T, Linnartz H, Chuang KJ.   +4 more
europepmc   +1 more source

Synchrotron FTIR Examination of Interplanetary Dust Particles: An Effort to Determine the Compounds and Minerals in Interstellar and Circumstellar Dust

, 2002
G. J. Flynn, L. P. Keller
openalex   +1 more source

Analysis of the interstellar dust polarized emission with the Planck Satellite Survey data

, 2015
Dana Alina
openalex   +1 more source

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Interstellar dust and extinction

Annual Review of Astronomy and Astrophysics, 1987
The ultraviolet (UV) region of the spectrum has been crucial in providing information on the nature of the material and size distribution of the particles of interstellar dust. Before there were any measurements of the UV properties of interstellar extinction, interstellar particles were believed to be composed primarily of dirty ices.
J. Mathis
semanticscholar   +2 more sources

Interstellar Dust

Interstellar and Intergalactic Medium, 2021

semanticscholar   +2 more sources

Interstellar Dust Grain Alignment

Annual Review of Astronomy and Astrophysics, 2015
Interstellar polarization at optical-to-infrared wavelengths is known to arise from asymmetric dust grains aligned with the magnetic field. This effect provides a potentially powerful probe of magnetic field structure and strength if the details of the grain alignment can be reliably understood.
B. Andersson, A. Lazarian, J. Vaillancourt   +2 more
semanticscholar   +2 more sources