WR 155 and its Surrounding ISM: Where Is the Bubble?

Details WR 155 and its Surrounding ISM: Where Is the Bubble? WR 155 and its Surrounding ISM: Where Is the Bubble?

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33..165n&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

Scientific paper

Stellar winds of massive stars seem rarely to leave easily identifiable and explained dynamical imprints on the surrounding interstellar medium. The sensible, classically-predicted wind bubbles are few and far between. As part of a concerted effort to solve the puzzle that this presents, we carefully investigate the gas and dust environment of the Wolf-Rayet star WR155. An arc of material seen in ^{12}CO data, faintly in infrared images, and more faintly yet in the HI images is the most likely signpost of the star's interaction with its environment.

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