Gaseous self gravitational effects in the aggregation of giant molecular clouds and the stability of global spiral structures.

Details Gaseous self gravitational effects in the aggregation of giant molecular clouds and the stability of global spiral structures. Gaseous self gravitational effects in the aggregation of giant molecular clouds and the stability of global spiral structures.

Jun 1988

adsabs.harvard.edu/abs/1988nastm4041..105r

NASA Tech. Memo., NASA TM-4041, p. 105

Physics

Interstellar Clouds:Spiral Structure, Spiral Galaxies:Spiral Structure

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