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Monte Carlo radiative transfer for the nebular phase of type Ia supernovae

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ABSTRACT. We extend the range of validity of the artis 3D radiative transfer code up to hundreds of days after explosion, when Type Ia supernovae (SNe Ia) are

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Bibliographic Details
Main Authors: Shingles, Luke J. (Author) , Kromer, Markus (Author) , Röpke, Friedrich (Author)
Format: Article (Journal)
Language:English
Published: 2020
In: Monthly notices of the Royal Astronomical Society
Year: 2020, Volume: 492, Issue: 2, Pages: 2029-2043
ISSN:1365-2966
DOI:10.1093/mnras/stz3412
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/stz3412
Verlag: https://academic.oup.com/mnras/article/492/2/2029/5691340
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Author Notes:L.J. Shingles, S.A. Sim, M. Kromer, K. Maguire, M. Bulla, C. Collins, C.P. Ballance, A.S. Michel, C.A. Ramsbottom, F.K. Röpke, I.R. Seitenzahl and N.B. Tyndall
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Summary:ABSTRACT. We extend the range of validity of the artis 3D radiative transfer code up to hundreds of days after explosion, when Type Ia supernovae (SNe Ia) are
Item Description:Advance access publication 2019 December 31
Gesehen am 17.02.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz3412

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