A new clue to the transition mechanism between optical high and low states of the supersoft X-ray source RX J0513.9-6951, implied by the recurrent nova CI aquilae 2000 outburst model

Astrophysical Journal

Volumn 588, Issue 2 I, 2003, Pages 1003-1008

  Hachisu, Izumi ^a   Kato, Mariko ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b KEIO UNIVERSITY   (Japan)

Author keywords

Binaries: close; Novae, cataclysmic variables; Stars : individual (CI Aquilae, RX J0513.9 6951); Stars: winds, outflows; X rays: stars

Indexed keywords

EID: 0041760776     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/374303     Document Type: Article

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