ROSAT observations of the RSCVn binary o Geminorum
Received 22 December 1995 / Accepted 2 March 1996
X-ray observations of the RSCVn system Geminorum have been undertaken with the ROSAT observatory. Several spectra of very good signal-to-noise ratio were obtained. Spectral fitting using metal abundances amounting to 50% of solar values reveal two temperature components at 2 MK and 12 MK. Previous EXOSAT observations showed another component at 40 MK. Particular interest is focused on the temporal variations of the X-ray emission. It is found that variations occur on time scales ranging from years to hours and minutes.
Key words: stars: coronae X-rays: stars stars oe Gem
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© European Southern Observatory (ESO) 1997
Online publication: July 3, 1998