A model for the optical high state light curve of AM Herculis

Astronomy and Astrophysics

Volumn 372, Issue 2, 2001, Pages 557-562

  Gansicke B T ^a   Fischer, A ^a   Silvotti, R ^b   De Martino, D ^b  

^a UNIVERSITY OF GÖTTINGEN   (Germany)

^b Osservatorio di Capodimonte   (Italy)

Author keywords

Accretion; Novae, cataclysmic variables; Stars: binaries close; Stars: individual: AM Her; Stars: white dwarfs

Indexed keywords

EID: 0035373216     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010522     Document Type: Article

References (31)