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The soft and hard X-rays thermal emission from star cluster winds with a supernova explosion

  • Published:2015-05-08 Issue:3 Volume:450 Page:2799-2811
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:

Author:

Castellanos-Ramírez A.,Rodríguez-González A.,Esquivel A.,Toledo-Roy J. C.,Olivares J.,Velázquez P. F.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 8 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. A comprehensive hydrodynamical study of SB DEM L50: understanding off-centre SNe and soft X-ray luminosity;Monthly Notices of the Royal Astronomical Society;2023-10-05

2. Deciphering the Morphological Origins of X-shaped Radio Galaxies: Numerical Modeling of Backflow versus Jet Reorientation;The Astrophysical Journal Supplement Series;2023-09-22

3. Inside the core of a young massive star cluster: 3D MHD simulations;Monthly Notices of the Royal Astronomical Society;2022-09-26

4. X-ray and optical emission from large superbubbles including the stellar photoionization;Monthly Notices of the Royal Astronomical Society;2022-02-02

5. 3D MHD simulations of the supernova remnant CTB 109;Monthly Notices of the Royal Astronomical Society;2021-10-11
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