The X-ray spectral evolution of classical nova v1974 cygni 1992: A re analysis of the rosat data

Astrophysical Journal

Volumn 499, Issue 1 PART I, 1998, Pages 395-406

  Balman, Solen ^a   Krauttfr, Joachim ^b   Ogelman, Hakki ^c  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b UNIVERSITÄT HEIDELBERG   (Germany)

^c University of Wisconsin Madison   (United States)

Author keywords

Binaries: close; Novae, cataclysmic variables; Radiation mechanisms: thermal stars: abundances; Stars: individual (Nova V1974 Cygni); X rays: stars

Indexed keywords

EID: 22044458336     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/305600     Document Type: Article

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