Results 111 to 120 of about 219,513 (216)
Unusual relative strengths of the diffuse interstellar bands in some interstellar dust clouds [PDF]
, 1986 Some of the diffuse interstellar features (DIBs) in the spectra of certain stars at high galactic latitudes (1 is greater than 15 degrees) are unusually weak or absent while others have the strength expected for their color excess.
Walker, G. A. H., Krelowski, J.
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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
Ultraviolet Interstellar Extinction toward High Galactic Latitudes
The Astrophysical JournalNearby high Galactic latitude clouds provide a unique laboratory to study the physics and structure of the Galactic interstellar medium and the properties of the interstellar dust.
Ajay Mishra, Aigen Li
doaj +1 more source
Radiative transfer and chemistry in spheroidal interstellar clouds
, 2002 The thesis begins by describing the way in which gas phase chemistry of the interstellar medium can be modelled, and demonstrating the potential significance of chemical reactions on the surfaces of dust grains present in the gas. The dust also serves as
O'Neill, Philip Thomas
core
The Astronomical JournalStrottner–Drechsler–Sainty Object 1 (SDSO1) is a faint [O iii ] emission nebula spanning 1 $\mathop{.}\limits^{^\circ }5$ , discovered southeast of M31.
Tiantian Liang +18 more
doaj +1 more source
A Pan-galaxy Study of Synthetic Giant Molecular Filaments: A Turbulence-dominated Life Cycle
The Astrophysical Journal Supplement SeriesRecent surveys of the Galactic plane have revealed dozens of giant molecular filaments (GMFs), with lengths ranging from tens to hundreds of parsecs, yet their origins and life cycles remain debated. In this work, we analyze over 700 GMFs identified from
Zipeng Hu +3 more
doaj +1 more source
Does the H+5 hydrogen cluster exist in dense interstellar clouds?
, 2012 The clustering of hydrogen molecules around a cation in dense interstellar clouds is examined taking into account recent accurate information about the structure and thermochemistry of these clusters.
Nascimento, M., Barbatti, M.
core +1 more source
The Young Ages of 70 μm Dark Clumps Inferred from Carbon Chain Chemistry
The Astrophysical JournalThe physical conditions of the earliest environment of high-mass star formation are currently poorly understood. To that end, we present observations of the carbon chain molecules HC _5 N, CCS, and HC _7 N in the 22–25 GHz band toward 12 high-mass 70 μ m
Kadin Worthen +6 more
doaj +1 more source
Pathway to the identification of C60+ in diffuse interstellar clouds. [PDF]
Philos Trans A Math Phys Eng Sci, 2016 Maier JP, Campbell EK.
europepmc +1 more source
Non-equilibrium ionization around clouds evaporating in the interstellar medium [PDF]
, 1986 It is of prime importance for global models of the interstellar medium to know whether dense clouds do or do not evaporate in the hot coronal gas. The rate of mass exchanges between phases depends very much on that.
Mora, P., Luciani, J. F., Ballet, J.
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