On the relation between supersoft X-ray sources and VY Scl stars: The cases of V504 Cen and VY Scl
J. Greiner (MPE Garching), R. Schwarz (AIP Potsdam), C. Tappert (Uni, de Valparaiso), R.E. Mennickent (Uni de de Concepcion), K. Reinsch (Uni, Goettingen), G. Sala (Univ. Politec. de Catalunya)
TL;DR
This paper investigates the connection between supersoft X-ray sources and VY Scl stars by monitoring V504 Cen and VY Scl during their state transitions using optical and X-ray observations.
Contribution
It provides new observational data on VY Scl stars during state transitions, exploring their relation to supersoft X-ray sources.
Findings
Optical monitoring captured state transitions of V504 Cen and VY Scl.
Triggered X-ray observations revealed supersoft X-ray emission during certain states.
The study suggests a link between VY Scl star behavior and supersoft X-ray phenomena.
Abstract
We summarize our optical monitoring program of VY Scl stars with the SMARTS telescopes, and triggered X-ray as well as optical observations after/during state transitions of V504 Cen and VY Scl.
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