X-ray and optical variations in the classical Be star γ Cassiopeia: The discovery of a possible magnetic dynamo

Astrophysical Journal

Volumn 575, Issue 1 I, 2002, Pages 435-448

  Robinson, Richard D ^a,b,c   Smith, Myron A ^a,b,d   Henry, Gregory W ^e  

^a Computer Sciences Corporation ^*  (United States)

^b CATHOLIC UNIVERSITY OF AMERICA   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d STScI   (United States)

^e TENNESSEE STATE UNIVERSITY   (United States)

Author keywords

Circumstellar matter; Line, Be; Stars: emission; Stars: flare; Stars: individual ( Cassiopeiae); Ultraviolet: stars; X rays: stars

Indexed keywords

EID: 0043234661     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/341141     Document Type: Article

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