A neutral hydrogen bipole associated with UW CMa

Details A neutral hydrogen bipole associated with UW CMa A neutral hydrogen bipole associated with UW CMa

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.221..707d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 221, Aug. 1, 1986, p. 707-713.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Eclipsing Binary Stars, Hydrogen Clouds, Neutral Gases, Astronomical Spectroscopy, Early Stars, O Stars, Velocity Distribution

Scientific paper

During a recent study of features associated with early-type stars, the
authors have observed a linearly extended, low-mass (180 M_sun;) cloud
of neutral hydrogen in the vicinity of UW CMa. The structure of this
cloud and its velocity field suggest that it is indeed associated with
UW CMa. Possible models for their relation are considered.

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