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Typical Scales of Structures in Numerical Models of Betelgeuse
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2002 (English)In: Modelling of Stellar Atmospheres, IAU Symposium 210, San Francisco: The Astronomical Society of the Pacific , 2002Conference paper, Published paper (Other scientific)
Abstract [en]

3D radiation hydrodynamics simulations of the envelope and atmosphere of a red supergiant show giant convection cells with sometimes deep-reaching downdrafts. Smaller short-lived cells can appear in the very outer layers. The surface intensity pattern is

Place, publisher, year, edition, pages
San Francisco: The Astronomical Society of the Pacific , 2002.
Series
IAU Symposia
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-44828OAI: oai:DiVA.org:uu-44828DiVA: diva2:72734
Note
Proceedings of IAU Symposium 210, held 17-21 June 2002 in Uppsala, SwedenAvailable from: 2008-10-17 Created: 2008-10-17

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