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Hydrodynamical simulations and similarity relations for eruptive mass-loss from massive stars

Abstract. Motivated by the eruptive mass-loss inferred from Luminous Blue Variable (LBV) stars, we present 1D hydrodynamical simulations of the response from s

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Bibliographic Details
Main Authors: Owocki, Stanley P. (Author) , Schneider, Fabian (Author)
Format: Article (Journal)
Language:English
Published: 2019 February 18
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 485, Issue: 1, Pages: 988-1000
ISSN:1365-2966
DOI:10.1093/mnras/stz461
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stz461
Verlag, Volltext: https://academic.oup.com/mnras/article/485/1/988/5333346
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Author Notes:Stanley P. Owocki, Ryosuke Hirai, Philipp Podsiadlowski and Fabian R.N. Schneider
Description
Summary:Abstract. Motivated by the eruptive mass-loss inferred from Luminous Blue Variable (LBV) stars, we present 1D hydrodynamical simulations of the response from s
Item Description:Gesehen am 13.03.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz461

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