CO observations of dark clouds in Lupus

Details CO observations of dark clouds in Lupus CO observations of dark clouds in Lupus

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...167..234m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 167, Oct. 1986, p. 234-238.

Astronomy and Astrophysics

Astrophysics

56

Carbon Monoxide, Interstellar Matter, Molecular Clouds, Molecular Spectra, Star Clusters, Extrasolar Planets, Herbig-Haro Objects, Radio Spectra, Star Formation, T Tauri Stars

Scientific paper

12CO observations covering 170 square degrees toward the southern T association Lupus have revealed the presence of an extended physically related complex of dark clouds which have recently formed low mass stars. The estimated mass of the clouds (≡3×104M_sun;) is comparable to that of the nearby Ophiuchus dust clouds. The Lupus clouds are projected onto a gap between two subgroups of the Scorpio-Centaurus OB association suggesting that this long accepted subgrouping may require reinterpretation.

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