@inproceedings{oai:jaxa.repo.nii.ac.jp:00005260,
 author = {武井, 大 and 辻本, 匡弘 and 北本, 俊二 and 村上, 弘志 and Takei, Dai and Tsujimoto, Masahiro and Drake, Jeremy and Ness, Jan-Uwe and Kitamoto, Shunji and Murakami, Hiroshi},
 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), We conducted target of opportunity X-ray observations of the classical novae V458 Vulpeculae and V2491 Cygni using the Suzaku satellite. With a short exposure of ca. 20 ks each, we obtained well-exposed spectra, enriching unique data sets of the shock X-ray emission from classical novae. V458 Vulpeculae shows lots of emission lines with a ca. 1 keV plasma temperature, while V2491 Cygni shows an emission line from Fe with a ca. 3 keV plasma temperature and a hard X-ray component. We report the results of these observations in this proceedings., Physical characteristics: Original contains color illustrations, 資料番号: AA0064306021, レポート番号: JAXA-SP-08-014E},
 pages = {100--101},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {X-ray study of classical novae: V458 Vul and V2491 Cyg},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}