SN1987Aから期待されるX線とぎんがによって観測されたX線(基研短期研究会「SN1987A」,研究会報告)

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概要

• 論文の詳細を見る

• The X-ray light curve and spectrum from SN 1987A due to Compton degradation of γ-rays from the ^<56>Co decay are calculated and compared with the Ginga and Kvant observations. If mixing of ^<56>Co into outer layers has taken place, the X-rays emerge much earlier than in the case without mixing and the resulting hard X-rays are in reasonable agreement with observations.

• 素粒子論グループ 素粒子研究編集部の論文
• 1988-05-20

著者

• NISHIMURA J.

  Institute of Space and Astronautical Science

• 熊谷 紫麻見

  Department Of Earth Science And Astronomy University Of Tokyo

• Itoh M.

  Institute of Space and Astronautical Science

• Shigeyama T.

  Department of Earth Science and Astronomy, University of Tokyo

• Nomoto K.

  Department of Earth Science and Astronomy, University of Tokyo

• Shigeyama T

  Univ. Tokyo Tokyo Jpn

• Shigeyama T.

  Department Of Astronomy Faculty Of Science University Of Tokyo:max-planck-institut Fur Physik Und As

• Nomoto K.

  Department Of Earth Science And Astronomy University Of Tokyo

• Nomoto K.

  Department Of Astronomy Faculty Of Science University Of Tokyo:max-planck-institut Fur Physik Und As

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