Interacting supernovae from photoionization-confined shells around red supergiant stars-Reference-Cited by-同舟云学术

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Interacting supernovae from photoionization-confined shells around red supergiant stars

Published:2014-08-10 Issue:7514 Volume:512 Page:282-285
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Mackey Jonathan,Mohamed Shazrene,Gvaramadze Vasilii V.,Kotak Rubina,Langer Norbert,Meyer Dominique M.-A.,Moriya Takashi J.,Neilson Hilding R.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

https://www.nature.com/articles/nature13522.pdf

Reference46 articles.

1. Noriega-Crespo, A., van Buren, D., Cao, Y. & Dgani, R. A parsec-size bow shock around Betelgeuse. Astron. J. 114, 837–840 (1997)

2. Ueta, T. et al. AKARI/FIS mapping of the ISM-wind bow shock around α Orionis. Pub. Astron. Soc. Jpn 60, S407–S413 (2008)

3. Mohamed, S., Mackey, J. & Langer, N. 3D simulations of Betelgeuse’s bow shock. Astron. Astrophys. 541, A1 (2012)

4. Decin, L. et al. The enigmatic nature of the circumstellar envelope and bow shock surrounding Betelgeuse as revealed by Herschel. I. Evidence of clumps, multiple arcs, and a linear bar-like structure. Astron. Astrophys. 548, A113 (2012)

5. Le Bertre, T., Matthews, L. D., Gérard, E. & Libert, Y. Discovery of a detached H I gas shell surrounding α Orionis. Mon. Not. R. Astron. Soc. 422, 3433–3443 (2012)

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