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

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
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

Models for type Ia supernovae and related astrophysical transients by Röpke, Friedrich (Author) , Sim, Stuart (Author) ,

in: Space science reviews, 214 (2018,4) Artikel-Nummer 72, 17 Seiten

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Article (Journal) Online Resource

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

Models for type Ia supernovae and related astrophysical transients by Röpke, Friedrich (Author) , Sim, Stuart (Author) ,

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