The cooling white dwarf in VW hydri after normal outburst and superoutburst: HST evidence of a sustained accretion belt

Astrophysical Journal

Volumn 471, Issue 1 PART II, 1996, Pages

  Sion, Edward M ^a   Cheng, F U Hua ^b   Huang, Min ^a   Hubeny, Ivan ^b,c   Szkody, Paula ^a,d  

^a VILLANOVA UNIVERSITY   (United States)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d UNIVERSITY OF WASHINGTON   (United States)

Author keywords

Novae, cataclysmic variables; Stars: Individual (vw hydri); White dwarfs

Indexed keywords

EID: 21444450412     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/310318     Document Type: Article

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