http://arxiv.org/abs/2303.14135
A novel method is presented which can pin down the time the accretion disk re-established itself in the RS Oph system after it experienced a nova disruption. The method is based on the re-ionisation of the ejecta by photoionisation from the radiation released in the boundary layer from accretion.
A. Azzollini, S. Shore and P. Kuin
Mon, 27 Mar 23
36/59
Comments: 3 pages, 1 figure
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