@inproceedings{oai:jaxa.repo.nii.ac.jp:00005256,
 author = {海老沢, 研 and Ebisawa, Ken},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop},
 month = {Feb},
 note = {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},
 pages = {82--85},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Galactic transient sources with MAXI},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}