Issue |
A&A
Volume 454, Number 1, July IV 2006
|
|
---|---|---|
Page(s) | 295 - 299 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20052989 | |
Published online | 03 July 2006 |
The RS CVn binary HK Lacertae: long-term photometry from Sonneberg sky-patrol plates
1
Astrophysikalisches Institut Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany e-mail: [hefroehlich;kstrassmeier]@aip.de
2
Sternwarte Sonneberg, Sternwartestr. 32, 96515 Sonneberg, Germany e-mail: pk@4pisysteme.de
Received:
4
March
2005
Accepted:
14
March
2006
Long-term photographic photometry of the active long-period RS CVn binary HK Lac (HD 209813) was obtained from more than 2000 Sonneberg Sky-Patrol plates
taken between 1956 and 1996. We achieve an internal accuracy of 0 07. The
correspondence with contemporaneous high-precision photoelectric photometry
from automatic telescopes is striking and successfully demonstrates the
feasibility of our approach. Based on a Bayesian time series analysis, we
improve the previously published cycle period to
years,
and present evidence of an additional period of
years. This establishes the multi-periodicity of dynamo action in these
overactive stars as compared to the Sun. The already known 6.7-years cycle
turns out to be
an overtone of the dominating 13.4-years cycle. Our long-term photographic
photometry even allowed the detection of the star's mean rotational period of
24.35 days.
Key words: stars: activity / stars: individual: HK Lacertae / stars: late-type / stars: rotation / stars: starspots
© ESO, 2006
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.