X-ray imaging of the Cr and Fe lines from Cassiopeia A

Open Access
Authors
  • Y. Maeda
  • T. Sato
  • H. Tsunemi
  • A. Bamba
  • J. Vink
  • Y. Terada
  • T. Takeda
  • M. Sawada
  • P. Gandhi
  • H. Matsumoto
  • Y. Uchiyama
  • E.A. Helder
  • J. Hiraga
  • J.P. Hughes
  • M. Kokubun
  • T. Tamagawa
  • Y. Tsuboi
Publication date 2014
Host editors
  • M. Ishida
  • R. Petre
  • K. Mitsuda
Book title Proceedings of Suzaku-MAXI 2014: Expanding the Frontiers of the X-ray Universe: February 19-22, 2014, Ehime University, Japan
Event Suzaku-MAXI 2014: Expanding the Frontiers of the X-ray Universe
Pages (from-to) 174-175
Publisher Matsuyama, Ehime Japan: Ehime University
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract Follow-up Suzaku X-ray observations of a young supernova remnant Cassiopeia A carried out with a long exposure of ˜ 165 ksec in 2012. Owing to the high statistics of the data, the map of Cr-K line is made. The flux map of Cr-K line is similar to that of Fe-K. The similarity indicates that the reverse shock is currently heating the electra layer that the Fe and Cr elements co-exists in
Document type Conference contribution
Language English
Published at http://wwwxray.ess.sci.osaka-u.ac.jp/SuzakuMAXI2014/proceedings.html
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X-ray imaging of the Cr (Final published version)
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