Results 71 to 80 of about 3,905 (166)
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
doaj +1 more source
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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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 Smallest Sizes of Diffuse Interstellar Clouds [PDF]
J. M. Dickey, J. Crovisier, I. Kazès
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A sequential acid-base (SAB) mechanism in the interstellar medium: The emergence of cis formic acid in dark molecular clouds [PDF]
Juan García de la Concepción +7 more
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ORTHO-H 2 AND THE AGE OF INTERSTELLAR DARK CLOUDS [PDF]
L. Pagani, E. Roueff, P. Lesaffre
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Modeling the Far-infrared Polarization Spectrum of a High-mass Star-forming Cloud
The polarization spectrum, or wavelength dependence of the polarization fraction, of interstellar dust emission provides important insights into the grain alignment mechanism of interstellar dust grains.
Dennis Lee +9 more
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