Implications of Collisionally-Supported Giant Molecular Clouds for Spiral Structure and Star Formation

Details Implications of Collisionally-Supported Giant Molecular Clouds for Spiral Structure and Star Formation Implications of Collisionally-Supported Giant Molecular Clouds for Spiral Structure and Star Formation

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baas...14..662l&link_type=gif

Bulletin of the American Astronomical Society, Vol. 14, p.662

Astronomy and Astrophysics

Astronomy

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