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2003ApJ...588.1003H - Astrophys. J., 588, 1003-1008 (2003/May-2)
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.
HACHISU I. and KATO M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Stars: Binaries: Close - Stars: Novae, Cataclysmic Variables - Stars: Individual: Constellation Name: CI Aquilae - Stars: Individual: Alphanumeric: RX J0513.9-6951 - Stars: Winds, Outflows - X-Rays: Stars
Simbad objects: 5
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