Structure and dynamics of the BOK globule B335

Details Structure and dynamics of the BOK globule B335 Structure and dynamics of the BOK globule B335

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icar...61...22f&link_type=abstract

(Conference on Protostars and Planets II, Tucson, AZ, Jan. 4-7, 1984) Icarus (ISSN 0019-1035), vol. 61, Jan. 1985, p. 22-26. NAS

Astronomy and Astrophysics

Astronomy

6

Carbon Monoxide, Interstellar Matter, Molecular Clouds, Angular Velocity, Astronomical Maps, Gas Density, Mass Distribution, Rotating Matter

Scientific paper

CO maps of the Bok globule B335 are presented and used to derive its density profile, mass distribution, and rotational velocity structure. It is found that the cloud is in nearly hydrostatic equilibrium with a density profile that varies roughly as r-1 in the core and r-3 in the envelope. The observed rotation is unimportant in the force balance at the present stage of evolution.

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