On the Possibility of Particle Acceleration in Shock Waves in WR Nebulae-Reference-Cited by-同舟云学术

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On the Possibility of Particle Acceleration in Shock Waves in WR Nebulae

Published:2018-11-03 Issue:4 Volume:61 Page:469-482
ISSN:0571-7256
Container-title:Astrophysics
language:en
Short-container-title:Astrophysics

Author:

Yeghikyan A.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://link.springer.com/article/10.1007/s10511-018-9551-8/fulltext.html

Reference41 articles.

1. L. Drury, Rep. Prog. Phys. 46, 973 (1983).

2. A. Reimer, M. Pohl, and O. Reimer, Astrophys. J. 644, 1118 (2006).

3. A. Yeghikyan and H. Fahr, Astron. Astrophys. submitted (2017).

4. A. Moffat, in: W.-R. Hamann, A. Sander, and H. Todt, ed., Wolf-Rayet Star, Potsdam, Univ. Verlag (2015), p. 13.

5. J. Toalá, A. Marston, M. Guerrero, et al., Astrophys. J. 846, 76 (2017).

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The irreplaceable role of ubiquitous cosmic rays in the space chemistry: from the origin of complex species in interstellar molecular clouds to the ozone depletion in the atmospheres of Earth-like planets;Communications of the Byurakan Astrophysical Observatory;2020

2. WR galaxies and PAH: observations and modeling;Communications of the Byurakan Astrophysical Observatory;2018

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