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  Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics

Noebauer, U. M., & Sim, S. A. (2015). Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics. Monthly Notices of the Royal Astronomical Society, 453(3), 3120-3134. doi:10.1093/mnras/stv1849.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0029-2193-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0029-2194-7
Genre: Journal Article

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 Creators:
Noebauer, U. M.1, Author              
Sim, S. A., Author
Affiliations:
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882              

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Language(s): eng - English
 Dates: 2015-11-01
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1093/mnras/stv1849
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. R. Astr. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 453 (3) Sequence Number: - Start / End Page: 3120 - 3134 Identifier: ISSN: 0035-8711