The ISM around southern O-type stars

Details The ISM around southern O-type stars The ISM around southern O-type stars

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33..164m&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

2

Ism: Bubbles, Hii Regions, Stars: Wolf-Rayet

Scientific paper

The structure and kinematics of the interstellar medium (ISM) are
strongly modified by the action of stellar winds from massive stars
which create interstellar bubbles. These structures can be detected as
slowly expanding neutral shells in the HIemission distribution around O
and WR stars (e.g. Cappa & Benaglia 1998; Cappa 2006).

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