The recurrent nova RS Oph: A possible scenario for type Ia supernovae

New Astronomy Reviews

Volumn 52, Issue 7-10, 2008, Pages 386-389

  Hernanz, M ^a,c   Jose J ^b,c  

^a UNIVERSITAT AUTÒNOMA DE BARCELONA   (Spain)

^b UNIVERSITAT POLITÈCNICA DE CATALUNYA   (Spain)

^c INSTITUT D ESTUDIS ESPACIALS DE CATALUNYA IEEC   (Spain)

Author keywords

Binaries; Cataclysmic variables; Close; Gamma ray astronomy; General; Individual (RS Oph); Novae; Nucleosynthesis; Stars; Supernovae; Symbiotic

Indexed keywords

EID: 51649101507     PISSN: 13876473     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.newar.2008.06.017     Document Type: Short Survey

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