| Author | Search for: Knee, L.; Search for: Wallace, W.1 |
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| Affiliation | - National Research Council of Canada. NRC Institute for Aerospace Research
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| Format | Text, Article |
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| Subject | ISM: bubbles; ISM: kinematics and dynamics; stars: winds, out-flows; stars: early-type; stars: Wolf-Rayet |
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| Abstract | 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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| Publication date | 2003 |
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| Publisher | Instituto de Astronomía México |
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| In | |
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| NPARC number | 9720675 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 1b8abcd6-f5ba-4318-aeb5-03eab90dcd34 |
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| Record created | 2009-07-17 |
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| Record modified | 2022-10-28 |
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