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arxiv 2303.14135 v1 pith:VEXD6EEP submitted 2023-03-14 astro-ph.HE astro-ph.SR

Spectroscopic Signature of a Re-established Accretion Disk in Symbiotic-like Recurrent Nova RS Ophiuchi

classification astro-ph.HE astro-ph.SR
keywords accretiondiskmethodnovare-establishedboundarydisruptiondown
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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.

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