A 2.8-second quasi-coherent oscillation in the soft X-ray flux of the dwarf nova SS Cygni

Astronomy and Astrophysics

Volumn 324, Issue 3, 1997, Pages

  Van Teeseling, André ^a  

^a UNIVERSITY OF GÖTTINGEN   (Germany)

Author keywords

Accretion disks; Cataclysmic variables; Oscillations; SS Cygni; Stars: individual; White dwarfs; X rays: stars

Indexed keywords

EID: 0008546741     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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