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

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

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

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 545
  • Basım Tarihi: 2012
  • Doi Numarası: 10.1051/0004-6361/201219681
  • Dergi Adı: ASTRONOMY & ASTROPHYSICS
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Anahtar Kelimeler: 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
  • Orta Doğu Teknik Üniversitesi Adresli: Evet

Özet

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.