3D radiative transfer simulations of Eta Carinae's inner colliding winds - I. Ionization structure of helium at apastron

Abstract. The highly eccentric binary system Eta Carinae (η Car) shows numerous time-variable emission and absorption features. These observational signatures a

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Bibliographic Details
Main Authors: Clementel, Nicola (Author) , Madura, T. I. (Author) , Kruip, C. J. H. (Author) , Paardekooper, Jan-Pieter (Author) , Gull, T. R. (Author)
Format: Article (Journal)
Language:English
Published: 08 January 2015
In: Monthly notices of the Royal Astronomical Society
Year: 2015, Volume: 447, Issue: 3, Pages: 2445-2458
ISSN:1365-2966
DOI:10.1093/mnras/stu2614
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stu2614
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/447/3/2445/2892768
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Author Notes:N. Clementel, T.I. Madura, C.J.H. Kruip, J.-P. Paardekooper and T.R. Gull
Description
Summary:Abstract. The highly eccentric binary system Eta Carinae (η Car) shows numerous time-variable emission and absorption features. These observational signatures a
Item Description:Gesehen am 01.12.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stu2614