ROSAT and AB Doradus: the first five years
نویسنده
چکیده
Five and a half years of data from an extensive ROSAT X-ray monitoring program devoted to the young Kstar AB Dor are presented. Begun in mid-1990, this program is aimed at the study of the long-term behaviour of coronal flux levels in this very active star. We compare the X-ray data with 17 years of V-band brightness monitoring that shows a 10-year decline between 1978 and 1989 and a subsequent rise phase. In contrast, the X-ray flux, which is very variable on time scales of minutes to weeks, exhibits no pronounced long-term trend over the 5 1/2 years of the program. This supports the concept of a saturated corona. Making use of the ROSAT all-sky survey data and data from the most extensive among the available pointed observationswe also discuss the short-term variablity in relation to the rotational time scale. We find evidence for a partial rotational modulation of the X-ray flux implying structural inhomogeneities in this saturated corona.
منابع مشابه
Simultaneous ORFEUS FUV and ROSAT X-ray observations of the young rapid rotator AB Doradus
We present simultaneous soft X-ray and FUV observations of the rapidly rotating young star AB Doradus (HD 36705), obtained with the position sensitive proportional counter (PSPC) on board ROSAT and the FUV/EUV spectrometer on board ORFEUS. The X-ray data show that AB Dor was in a high state, possibly in a flare, during the FUV observations. The lines of CIII at 977 Å and OVI at 1032 and 1038 Å ...
متن کاملDynamical masses of the low-mass stellar binary AB Doradus B
Context. AB Doradus is the main system of the AB Doradus moving group. It is a quadruple system formed by two widely separated binaries of pre-main-sequence (PMS) stars: AB Dor A/C and AB Dor Ba/Bb. The pair AB Dor A/C has been extensively studied and its dynamical masses have been determined with high precision, thus making AB Dor C a benchmark for calibrating PMS stellar models. If the orbit ...
متن کاملMagnetic activity on AB Doradus: Temporal evolution of starspots
Surface brightness maps for the young K0 dwarf AB Doradus are reconstructed from archival data sets for epochs spanning 1988 to 1994. By using the signal-to-noise enhancement technique of Least-Squares Deconvolution, our results show a greatly increased resolution of spot features than obtained in previously published surface brightness reconstructions. These images show that for the exception ...
متن کاملTwo X-ray Sources in 30 Doradus: Wolf-rayet + Black Hole Binaries?
I report the detection of two X-ray sources of luminosities ∼ 10 36 ergs s −1 in the central region of 30 Doradus. These two sources appear point-like in images taken with the ROSAT HRI. One of the sources is most likely associated with a close spectroscopic binary R140a2 (WN6) with an orbital period of 2.76 days. The mass of the unknown binary component is likely in the range of 2.4 − 15 M ⊙. ...
متن کاملModeling the Corona of Ab Doradus
We present a model for the coronal topology of the active, rapidly rotating K0 dwarf, AB Doradus. Surface magnetic field maps obtained using a technique based on Zeeman Doppler imaging indicate the presence of a strong non-potential component near the pole of the star. The coronal topology is obtained by extrapolating these surface maps. The temperature and density in the corona are evaluated u...
متن کامل