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Annual Review of Astronomy and Astrophysics, 1991
Molecular gas is critical in determining both the morphology and evolution of galactic disks. It is within the giant molecular clouds that interstellar gas is cycled into the next generation of stars, and the most massive of these young stars produce a major part of the galactic luminosity.
Young, JS, SCOVILLE, NZ
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Molecular gas is critical in determining both the morphology and evolution of galactic disks. It is within the giant molecular clouds that interstellar gas is cycled into the next generation of stars, and the most massive of these young stars produce a major part of the galactic luminosity.
Young, JS, SCOVILLE, NZ
openaire +3 more sources
Intense Condensation of a Molecular Gas
Fluid Dynamics, 1997zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Kuznetsova, I. A. +2 more
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