Apsidal motion in the eclipsing binary AS Camelopardalis
Astronomical Institute, Charles University Prague, CZ-150 00 Praha 5, Švédská 8, Czech Republic
2 Astronomical Institute, University Basel, CH-4102 Binningen, Venusstrasse 7, Switzerland
Corresponding author: Send offprint request to: M. Wolf; email@example.com
Accepted: 7 October 1995
We report several new reliable times of minimum of the eclipsing binary AS Cam. Using all precise timings found in the literature, the O-C diagram is analyzed and improved values for the elements of the apsidal motion are computed. The discrepancy between observed rotational velocity of the line of apsides and the theoretically expected value still remains unresolved.
Key words: binaries: eclipsing / stars: individual: AS Cam
© European Southern Observatory (ESO), 1996