Rosat observations of FK comae berenices

Alan D. Welty, Lawrence W. Ramsey

Research output: Contribution to journalArticle

8 Scopus citations

Abstract

We obtained ROSAT PSPC observations of FK Com over a period of 24.4 h, or 0.42 rotation. During the observations the x-ray flux increased by a factor of at least 5 before declining toward its previous level. A single temperature Raymond-Smith model is adequate to model the low signal-to-noise ratio spectrum from each observation interval. Initially the spectrum was that of a 8.5×106 K plasma, with LX=0.66×1031 erg s-1. When the x-ray flux was greatest, the model plasma temperature rose to 2.5×107 K, and LX=3.46×1031 erg s-1. During the post-maximum decline in luminosity the plasma temperature was ∼12×106 K. We conclude that the increase of x-ray flux recorded by ROSAT was due to an x-ray flare with a 1.5 h decline time scale.

Original languageEnglish (US)
Pages (from-to)299-303
Number of pages5
JournalAstronomical Journal
Volume108
Issue number1
DOIs
StatePublished - Jul 1994

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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