Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-05-28
Astronomy and Astrophysics
Astrophysics
6 pages, 4 figures, accepted for Astronomy and Astrophysics, May 2001
Scientific paper
10.1051/0004-6361:20010693
The active late-type star AB Doradus was observed in February 1996 with the Goddard High Resolution Spectrograph of the Hubble Space Telescope using the low resolution G140L grating. The observations covered one half of the star's rotation cycle (P = 0.514 d) with 11.5 min time resolution. The strong coronal Fe XXI 1354.094 line formed at 10^7 K was analysed and its emission measure (EM) derived. This EM is much higher than that derived from recent XMM-Newton observations (Guedel et al. 2001), and earlier EXOSAT (Collier Cameron et al. 1988) and ASCA/EUVE (Mewe et al. 1996) data, as well, requiring a variability by a factor of 5. The physical reason for the variability remains unknown, since (outside flares) the observed broad band variability of AB Dor is much smaller.
Hakala Pasi
Mewe Rolf
Muhli Panu
Vilhu Osmi
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