Identification of the fast, high galactic latitude X-ray transient A 0000 + 28 with the RS CVn system HD 224085

D. A. Schwartz, M. Garcia, E. Ralph, R. E. Doxsey, M. D. Johnston, A. Lawrence, I. M. McHardy, J. P. Pye

Research output: Contribution to journalArticlepeer-review

Abstract

We identify the fast, high galactic latitude X-ray transient A 0000+28 (=3A 2355+284) with HD 224085, a known RSCVn system. This strengthens the suggestion that RS CVn systems are responsible for a significant fraction of this class of X-ray transient. The hard X-ray flares provide further data relevant to the interpretation of these systems by analogy to solar phenomena.
Original languageEnglish
Pages (from-to)95-100
JournalMonthly Notices of the Royal Astronomical Society
Volume196
DOIs
Publication statusPublished - 1 Jul 1981

Keywords

  • Flare Stars
  • Stellar Luminosity
  • Stellar Radiation
  • X Ray Sources
  • Ariel 5 Satellite
  • Binary Stars
  • Light Curve
  • Stellar Coronas
  • X Ray Stars

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