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URN: urn:nbn:de:kobv:517-opus-17659
URL: http://opus.kobv.de/ubp/volltexte/2008/1765/
Smith, Nathan
Independent signs of lower mass-loss rates for O-type stars
Kurzfassung in Englisch
I discuss observational evidence – independent of the direct spectral diagnostics of stellar winds themselves – suggesting that mass-loss rates for O stars need to be revised downward by roughly a factor of three or more, in line with recent observed mass-loss rates for clumped winds. These independent constraints include the large observed mass-loss rates in LBV eruptions, the large masses of evolved massive stars like LBVs and WNH stars, WR stars in lower metallicity environments, observed rotation rates of massive stars at different metallicity, supernovae that seem to defy expectations of high mass-loss rates in stellar evolution, and other clues. I pay particular attention to the role of feedback that would result from higher mass-loss rates, driving the star to the Eddington limit too soon, and therefore making higher rates appear highly implausible. Some of these arguments by themselves may have more than one interpretation, but together they paint a consistent picture that steady line-driven winds of O-type stars have lower mass-loss rates and are significantly clumped.
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RVK - Regensburger Verbundklassifikation: |
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US 1999.07 |
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Collection 1: |
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Universität Potsdam / Tagungen / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007 |
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Collection 2: |
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Universität Potsdam / Tagungen / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007 / Talks and Discussions (in alphabetical order) |
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Collection 3: |
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Universität Potsdam / Tagungen / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007 / Talks and Discussions (organized by sections) / Spectroscopy and mass loss diagnostic: observations |
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Institut: |
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Extern |
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DDC-Sachgruppe: |
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Astronomie |
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Dokumentart: |
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c InProceedings (Aufsatz / Paper einer Konferenz etc.) |
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Sprache: |
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Englisch |
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Erstellungsjahr: |
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2007 |
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Publikationsdatum: |
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25.04.2008 |
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Bemerkung: |
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The complete edition of the proceedings "Clumping in hot-star winds" is available:
urn:nbn:de:kobv:517-opus-13981 |
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Lizenz: |
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