Interpreting the near-infrared spectra of the ‘golden standard’ Type Ia supernova 2005cf-Reference-Cited by-同舟云学术

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Interpreting the near-infrared spectra of the ‘golden standard’ Type Ia supernova 2005cf

Published:2012-11-05 Issue:2 Volume:427 Page:994-1003
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Gall E. E. E.¹,Taubenberger S.¹,Kromer M.¹,Sim S. A.²,Benetti S.³,Blanc G.,Elias-Rosa N.,Hillebrandt W.¹

Affiliation:

1. Max-Planck-Institut für Astrophysik; Karl-Schwarzschild-Str. 1; 85741; Garching bei München; Germany

2. Research School of Astronomy & Astrophysics; Mount Stromlo Observatory; Cotter Road; Weston; ACT; 2611; Australia

3. INAF Osservatorio Astronomico di Padova; Vicolo dell’Osservatorio 5; 35122; Padova; Italy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/427/2/994/3007309/427-2-994.pdf

Reference61 articles.

1. Supernova 2002bo: inadequacy of the single parameter description

2. The Diversity of Type Ia Supernovae: Evidence for Systematics?

3. Infrared and optical spectroscopy of Type Ia supernovae in the nebular phase

4. Accreting white dwarf models for the type I supernovae. IV The optical spectrum of a carbon-deflagration supernova

5. Comparative Direct Analysis of Type Ia Supernova Spectra. II. Maximum Light

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