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Detection of Highly-Ionized Carbon and Nitrogen Emission Lines from the Cygnus Loop Supernova Remnant with the Suzaku Observatory

  • Published:2007-01-30 Issue:sp1 Volume:59 Page:S163-S170
  • ISSN:0004-6264
  • Container-title:Publications of the Astronomical Society of Japan
  • language:en
  • Short-container-title:Publ Astron Soc Jpn

Author:

Miyata Emi,Katsuda Satoru,Tsunemi Hiroshi,Hughes John P.,Kokubun Motohide,Porter F. Scott

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 32 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. Middle-Aged and Old Supernova Remnants;Astronomy and Astrophysics Library;2020

2. The spectral response of X-ray CCDs in the energy band around Si-K edge: a solution to the Si-K edge problem for the XIS onboard Suzaku;High Energy, Optical, and Infrared Detectors for Astronomy VIII;2018-07-20

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

4. SOFT X-RAY SPECTROSCOPY OF THE CYGNUS LOOP SUPERNOVA REMNANT;The Astrophysical Journal;2013-03-06

5. Evolution of Supernova Remnants Expanding out of the Dense Circumstellar Matter into the Rarefied Interstellar Medium;Publications of the Astronomical Society of Japan;2012-04-25
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