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 |
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Pages (from-to) | 1077-1079 |
Number of pages | 3 |
Journal | Astronomische Nachrichten |
Volume | 331 |
Issue number | 9-10 |
DOIs | |
Publication status | Published - Dec 2010 |