The first resolved and detected classical nova shell in X-rays: The shell of Nova Persei 1901

Astrophysical Journal

Volumn 518, Issue 2 PART 2, 1999, Pages

  Balman, Şölen ^a,b   Ögelman, Hakki B ^b  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b Wisconsin Electric Machines and Power Electronics Consortium   (United States)

Author keywords

Binaries: close; Novae, cataclysmic variables; Radiation mechanisms: thermal; Stars: individual (GK Persei); X rays: stars

Indexed keywords

EID: 0040249055     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/312069     Document Type: Article

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