Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae-Reference-Cited by-同舟云学术

Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae

Published:2018-07-02 Issue:9 Volume:2 Page:731-736
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Hamaguchi Kenji^ORCID,Corcoran Michael F.,Pittard Julian M.^ORCID,Sharma Neetika,Takahashi Hiromitsu^ORCID,Russell Christopher M. P.,Grefenstette Brian W.,Wik Daniel R.,Gull Theodore R.,Richardson Noel D.,Madura Thomas I.,Moffat Anthony F. J.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-018-0505-1.pdf

Reference45 articles.

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2. Morlino, G. & Caprioli, D. Strong evidence for hadron acceleration in Tycho’s supernova remnant. Astron. Astrophys. 538, A81 (2012).

3. Pittard, J. M. & Dougherty, S. M. Radio, X-ray, and γ-ray emission models of the colliding-wind binary WR140. Mon. Not. R. Astron. Soc. 372, 801–826 (2006).

4. De Becker, M., Benaglia, P., Romero, G. E. & Peri, C. S. An investigation into the fraction of particle accelerators among colliding-wind binaries. Towards an extension of the catalogue. Astron. Astrophys. 600, A47 (2017).

5. Corcoran, M. F. X-ray monitoring of η Carinae: variations on a theme. Astron. J. 129, 2018–2025 (2005).

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