H I Tails from Molecular Clouds near HD 17603 and Wolf-Rayet 5

Details H I Tails from Molecular Clouds near HD 17603 and Wolf-Rayet 5 H I Tails from Molecular Clouds near HD 17603 and Wolf-Rayet 5

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...44k&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: Bubbles, Ism: Kinematics And Dynamics, Stars: Winds, Outflows, Stars: Early-Type, Stars: Wolf-Rayet

Scientific paper

We report the detection of long, thin H I tails emanating from molecular
clouds in the Perseus Arm of the Galaxy. The hypothesis that they are
driven by stellar winds from one or both of the massive stars HD 17603
and WR 5 places strong constraints on the stellar wind environment: we
find that a heavily mass-loaded wind bubble is required.

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