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3D numerical model for an asymmetrical superbubble
- Massive stars usually form groups such as OB associations. Their fast stellar winds sweep up collectively the surrounding insterstellar medium (ISM) to generate superbubbles. Observations suggest that superbubble evolution on the surrounding ISM can be very irregular. Numerical simulations considering these conditions could help to understand the evolution of these superbubbles and to clarify the dynamics of these objects as well as the difference between observed X-ray luminosities and the predicted ones by the standard model (Weaver et al. 1977).
Author details: | J. Reyes-Iturbide, P. Velázquez, M. Rosado |
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URN: | urn:nbn:de:kobv:517-opus-17724 |
Publication type: | Conference Proceeding |
Language: | English |
Publication year: | 2007 |
Publishing institution: | Universität Potsdam |
Release date: | 2008/04/25 |
RVK - Regensburg classification: | US 1999.07 |
Organizational units: | Extern / Extern |
DDC classification: | 5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften |
Collection(s): | Universität Potsdam / Tagungsbände/Proceedings (nicht fortlaufend) / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007 |
Universität Potsdam / Tagungsbände/Proceedings (nicht fortlaufend) / Clumping in hot-star winds: International Workshop, Potsdam, Germany, 18. - 22. June 2007 / Posters | |
License (German): | Keine öffentliche Lizenz: Unter Urheberrechtsschutz |
External remark: | The complete edition of the proceedings "Clumping in hot-star winds" is available: urn:nbn:de:kobv:517-opus-13981 |