Results 101 to 110 of about 789,439 (256)
Strength Ratios of Diffuse Interstellar Bands in Slightly Reddened Objects
The disk of the Milky Way fills the interstellar medium in the form of discrete clouds, many (∼30) light-years across. The average density of this medium is 1 hydrogen atom per cm3 (Oort limit), in the clouds—several dozen atoms, and between the clouds ...
Jacek Krełowski, Arkadii Bondar
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Magnetic Braking of Collapsing Interstellar Clouds [PDF]
Robert Fleck, James H. Hunter
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Interstellar clouds containing optically thick H2
The theory of Black and Delgarno that the relative populations of the excited rotational levels of H2 can be understood in terms of cascading following absorption in the Lyman and Werner bands is employed to infer the gas densities and radiation fields within diffuse interstellar clouds containing H2 that is optically thin in those bands.
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The Passage of the Solar System through the Edge of the Local Bubble
The Sun moves through the interstellar medium (ISM) at a velocity of ∼19 pc Myr ^−1 , making the conditions outside the solar system vary with time over millions of years.
Merav Opher +12 more
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The Formation of Large Hydrocarbons and Carbon Clusters in Dense Interstellar Clouds [PDF]
Ryan P. A. Bettens, Eric Herbst
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Evidence that Earth was exposed to Cold Dense Interstellar Medium 2 Myrs Ago as a result of the Encounter with Local Lynx Cold Clouds [PDF]
M. Opher, Abraham Loeb, J. E. G. Peek
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87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
3D Simulation of Interstellar Cloud Collision and Triggered Star Formation [PDF]
Mikio Nagasawa, Shoken M. Miyama
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Cloud-cloud collisions in the interstellar medium
Results are presented from time-dependent numerical simulations of cloud-cloud collisions in the interstellar medium. Special emphasis is placed on physically detailed models of cloud collisions. The numerical simulations include heating, cooling, thermal conductivity, self-gravity, and molecule formation; magnetic fields have been neglected.
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