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A&A 389, 202-212 (2002)
DOI: 10.1051/0004-6361:20020506
Doppler imaging of stellar surface structure
XVIII. The very active RS CVn binary UZ Librae revisited
K. Oláh1, K. G. Strassmeier2 and M. Weber21 Konkoly Observatory of the Hungarian Academy of Sciences, 1525 Budapest, Hungary
e-mail: olah@konkoly.hu
2 Astrophysical Institute Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
(Received 7 December 2001 / Accepted 3 April 2002)
Abstract
We present eight Doppler images of UZ Librae from the
years 1994, 1996, 1997, 1998 and 2000. These maps indicate a
preferred temperature distribution from one year to the other and
suggest preferred spot locations for at least the seven years of
our observations. Two equatorial active regions appear facing
towards and opposite the (unseen) companion star. A large and cool
polar spot, with two or maybe three appendages extending down to a
latitude of 40°-50°, is present and causes the
long-term light variability of UZ Lib. The appendages appear at
longitudes very similar to the two equatorial active regions and
sometimes are possibly even attached to them. No coherent sign of
differential rotation is found for the equatorial regions up to a
latitude of approximately +50°, but the polar appendages may
indicate a general acceleration of the polar regions. If
interpreted as being due to differential rotation, if real at
all, then UZ Lib clearly exhibits a non-solar flow
pattern.
Key words: starspots -- stars: activity -- stars: atmospheres -- stars: late-type -- stars: individual: UZ Lib -- stars: binaries: close
Offprint request: K. G. Strassmeier, Kstrassmeier@aip.de, Mweber@aip.de
SIMBAD Objects
© ESO 2002
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