The interstellar bubble around Theta MUSCAE

Details The interstellar bubble around Theta MUSCAE The interstellar bubble around Theta MUSCAE

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1398c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 89, Sept. 1984, p. 1398-1403.

Astronomy and Astrophysics

Astronomy

32

Astronomical Spectroscopy, Binary Stars, Hydrogen Clouds, Interstellar Matter, Nebulae, Wolf-Rayet Stars, Astronomical Maps, Centimeter Waves, Neutral Gases, Stellar Models, Stellar Winds, Visible Spectrum

Scientific paper

H I observations of the interstellar medium surrounding θ Mus are presented. They show the existence of a hole 100 pc in diameter in the neutral hydrogen distribution due to the action of the strong stellar wind of the WR star which produces an expanding bubble of swept-up ambient material. Using the observational parameters, the authors discuss kinematical models for the H I shell around the bubble, and find that only the momentum conserving model applies.

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