A solar-type star polluted by calcium-rich supernova ejecta inside the supernova remnant RCW 86-Reference-Cited by-同舟云学术

A solar-type star polluted by calcium-rich supernova ejecta inside the supernova remnant RCW 86

Published:2017-04-24 Issue:6 Volume:1 Page:
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Gvaramadze Vasilii V.,Langer Norbert,Fossati Luca^ORCID,Bock Douglas C.-J.,Castro Norberto,Georgiev Iskren Y.,Greiner Jochen,Johnston Simon,Rau Arne,Tauris Thomas M.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-017-0116.pdf

Reference50 articles.

1. González Hernández, J. I. et al. Chemical abundances of the secondary star in the black hole X-ray binary V404 Cygni. Astrophys. J. 738, 95 (2011).

2. Perets, H. B. et al. A faint type of supernova from a white dwarf with a helium-rich companion. Nature 465, 322–325 (2010).

3. Kasliwal, M. M. et al. Calcium-rich gap transients in the remote outskirts of galaxies. Astrophys. J. 755, 161 (2012).

4. Kawabata, K. S. et al. A massive star origin for an unusual helium-rich supernova in an elliptical galaxy. Nature 465, 326–328 (2010).

5. Waldman, R. et al. Helium shell detonations on low-mass white dwarfs as a possible explanation for SN 2005E. Astrophys. J. 738, 21 (2011).

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