Galactic transient sources with MAXI

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Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008)

Thanks to its superior sensitivity, energy resolution and wide energy coverage, MAXI is expected to open a new window in the study of Galactic X-ray transients. In this paper, I selected the following eight areas in which MAXI is expected to make significant contributions to our understanding of the Galactic transient sources: (1) Detailed study of bright transients, (2) Monitor spectral variations, (3) Accretion disk spectral variation, (4) Faint transients, (5) Transient search in crowded region, (6) Supergiant fast X-ray transients, (7) Ultra-soft transients, and (8) Extragalactic stellar transients. For each area, I explain what MAXI will be able to do, in contrast to previous observations by all sky monitors.

資料番号: AA0064306017

レポート番号: JAXA-SP-08-014E

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詳細情報 詳細情報について

  • CRID
    1050574036239274624
  • NII論文ID
    120006828725
  • NII書誌ID
    AA11984031
  • ISSN
    1349113X
  • Web Site
    http://id.nii.ac.jp/1696/00005250/
  • 本文言語コード
    en
  • 資料種別
    conference paper
  • データソース種別
    • IRDB
    • CiNii Articles

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