The outburst of Nova CSS 081007:030559+054715 (HV Ceti)

Creative Commons License

Beardmore A. P., Osborne J. P., Page K. L., Hakala P. J., Schwarz G. J., Rauch T., ...More

ASTRONOMY & ASTROPHYSICS, vol.545, 2012 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 545
  • Publication Date: 2012
  • Doi Number: 10.1051/0004-6361/201219681
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Keywords: novae, cataclysmic variables, stars: individual: CSS 081007: 030559+054715 (HV Cet), X-rays: stars, ultraviolet: stars, X-RAY SOURCE, LARGE-MAGELLANIC-CLOUD, ABUNDANCE ANALYSIS, LIGHT-CURVE, SWIFT OBSERVATIONS, MODEL ATMOSPHERES, SYSTEM PARAMETERS, AM-HERCULIS, NO. 2, SUPERSOFT
  • Middle East Technical University Affiliated: Yes


Aims. The outburst of nova CSS 081007:030559+054715 (HV Cet) was extensively followed by Swift to study the evolution of its X-ray and UV emission.