Giant molecular clouds in the outer arm of the galaxy

Details Giant molecular clouds in the outer arm of the galaxy Giant molecular clouds in the outer arm of the galaxy

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...357l..29d&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 357, July 10, 1990, p. L29-L33.

Other

56

H Ii Regions, Interstellar Gas, Milky Way Galaxy, Molecular Clouds, Carbon Monoxide, Luminosity, Spectral Line Width

Scientific paper

Giant molecular clouds in the outer arm of the Galaxy comparable in size and mass to the largest clouds in the inner Galaxy between R about 3 kpc and the solar circle have been detected in a new CO survey along the Galactic plane from l = 65 deg to 71 deg centered about b = + 1 deg. These objects at R about 12 kpc are underluminous in CO; the N(H2)/W(CO) ratio determined from either virial masses or the CO luminosity-line width relation is 4 + or - 2 times that in the inner Galaxy. When extrapolated to the entire Galaxy beyond R = 11 kpc, the present survey and related data yield a total molecular mass in the range (1-7) x 10 to the 8th solar masses. The outer arm complexes surveyed contain the two most luminous H II regions known beyond R about 10 kpc; one is the distant component of W58, and the other is a previously unidentified distant component of S98.

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