Suzaku detection of superhard X-ray emission from the classical Nova V2491 Cygni

Astrophysical Journal

Volumn 697, Issue 1 PART 2, 2009, Pages

  Takei, D ^a   Tsujimoto, M ^b,c   Kitamoto, S ^a   Ness, J U ^d,e   Drake, J J ^f   Takahashi, H ^g   Mukai, K ^h,i  

^a RIKKYO UNIVERSITY   (Japan)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c PENNSYLVANIA STATE UNIVERSITY   (United States)

^d ARIZONA STATE UNIVERSITY   (United States)

^e EUROPEAN SPACE AGENCY   (France)

^f SMITHSONIAN ASTROPHYSICAL OBSERVATORY   (United States)

^g HIROSHIMA UNIVERSITY   (Japan)

^h NASA GODDARD SPACE FLIGHT CENTER   (United States)

ⁱ UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

Author keywords

Novae, cataclysmic variables; Stars: individual (Nova Cygni 2008 number 2, V2491 Cygni); X rays: stars

Indexed keywords

EID: 67649180388     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/697/1/L54     Document Type: Article

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