Abstract
X-ray observations of the RSCVn system sigma 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.
Original language | English |
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Journal | Astronomy and Astrophysics |
Volume | 318 |
Issue number | 3 |
Pages (from-to) | 791-796 |
ISSN | 0004-6361 |
Publication status | Published - 1997 |
Keywords
- X-rays
- Coronae
- Stars sigma Gem
- Stars