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astro-ph.GAOct 2, 2009
9
citations (OpenAlex)
authors
  • J. Greiner
  • R. Schwarz
  • C. Tappert
  • R. E. Mennickent
  • K. Reinsch
  • G. Sala
institutions
  • Leibniz Institute for Astrophysics Potsdam
  • Max Planck Institute for Extraterrestrial Physics
  • Max Planck Society
  • Universitat Politècnica de Catalunya
  • University of Concepción
  • University of Göttingen
  • University of Valparaíso
arXiv abstractPDF
paper

On the relation between supersoft X-ray sources and VY Scl stars: The cases of V504 Cen and VY Scl

arXiv:0910.0475 · doi:10.1002/asna.200911332

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.

4 pages, Proc. of workshop "SuperSoft X-ray Sources - New Developments", ESTEC/Villafranca, May 2009, to appear in AN

References in corpus (1)

  • The Donor Stars of Cataclysmic Variables

Cited by in corpus (7)

  • A comparative study of the strength of flickering in cataclysmic variables
  • TESS light curves of cataclysmic variables I -- Unknown periods in long-known stars
  • The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and gamma-rays
  • X-ray observations of VY Scl type nova-like binaries in the high and low state
  • Optical and X-ray Properties of CAL 83: I. Quasi-periodic Optical and Supersoft Variability
  • Novalike Cataclysmic Variables in the Infrared
  • SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first year
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