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- W1610363462 abstract "X-ray observations of the flare-star binary system Gliese 867AB obtained with the Low Energy instrument on the EXOSAT Observatory, are analysed. By applying a likelihood method, it is shown that both components of the system were contributing to the observed X-ray emission with an intensity ratio A:B of about 3:1. It is also shown that X-ray flares with energies of the order of 10 32 erg originated from both stars. In the light of these EXOSAT results, previous X-ray observations made with the IPC instrument aboard the Einstein Observatory are reanalysed and it is found, somewhat unexpectedly, that during those observations G867B was roughly as bright as G867A." @default.
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- W1610363462 date "1991-01-01" @default.
- W1610363462 modified "2023-09-25" @default.
- W1610363462 title "Quiescent and flaring X-rays from both Gliese 867A and Gliese 867B" @default.
- W1610363462 hasPublicationYear "1991" @default.
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