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X-ray spectroscopy of the mixed morphology supernova remnant W 28 with XMM-Newton

  • Published:2014-06-01 Issue:3 Volume:66 Page:62-62
  • ISSN:0004-6264
  • Container-title:Publications of the Astronomical Society of Japan
  • language:en
  • Short-container-title:Publications of the Astronomical Society of Japan

Author:

Nakamura R.,Bamba A.,Ishida M.,Yamazaki R.,Tatematsu K.,Kohri K.,Puhlhofer G.,Wagner S. J.,Sawada M.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 14 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. Initial state of the recombining plasma in supernova remnant W 28;Publications of the Astronomical Society of Japan;2023-02-08

2. Searching for an interstellar medium association for HESS J1534 − 571;Monthly Notices of the Royal Astronomical Society;2018-07-06

3. Leaked GeV CRs from a Broken Shell: Explaining 9 Years of Fermi-LAT Data of SNR W28;The Astrophysical Journal;2018-06-13

4. The origin of recombining plasma and the detection of the Fe-K line in the supernova remnant W 28;Publications of the Astronomical Society of Japan;2018-03-22

5. The gas-to-extinction ratio and the gas distribution in the Galaxy;Monthly Notices of the Royal Astronomical Society;2017-06-23
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