Abstract
We present results of a photometric study of the young southern open cluster Stock 14. This cluster is known to contain two eclipsing systems with presumed β Cephei components, HD 101794 and HD 101838. We confirm variability due to pulsations and eclipses in both targets and announce the discovery of other variable stars in the observed field.
| Original language | English |
|---|---|
| Pages (from-to) | 1077-1079 |
| Number of pages | 3 |
| Journal | Astronomische Nachrichten |
| Volume | 331 |
| Issue number | 9-10 |
| DOIs | |
| Publication status | Published - Dec 2010 |
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