Variable stars in the field of the open cluster NGC 7789.
Abstract
Fifteen variable stars have been discovered during four nights of monitoring of NGC 7789. It was possible to determine periods for ten of these variables. Seven objects are W UMa-type binaries, in this number five are members of the cluster. Among the remaining variables, there are three further close binaries, one δ Scuti which is a blue straggler in the cluster, and one multi-modal variable (with indeterminable periods). One of the binaries showed an eclipse-like event; this binary is a good candidate for determination of masses of its components at the turn-off point of the cluster.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- March 1995
- DOI:
- 10.48550/arXiv.astro-ph/9410015
- arXiv:
- arXiv:astro-ph/9410015
- Bibcode:
- 1995A&A...295..101J
- Keywords:
-
- Color-Magnitude Diagram;
- Eclipsing Binary Stars;
- Periodic Variations;
- Star Clusters;
- Variable Stars;
- Astronomical Photometry;
- Chronology;
- Data Reduction;
- Light Curve;
- Metallicity;
- Red Shift;
- Astronomy;
- BINARIES: CLOSE;
- BINARIES: ECLIPSING;
- {DELTA} SCU;
- STARS: VARIABLES: OTHER;
- OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL NGC 7789;
- BLUE STRAGGLERS;
- Astrophysics
- E-Print:
- A&