Variable Stars in the Open Cluster M29

Details Variable Stars in the Open Cluster M29 Variable Stars in the Open Cluster M29

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jkas...29...31k&link_type=abstract

Journal of the Korean Astronomical Society, vol. 29, no. 1, p. 31-41

Astronomy and Astrophysics

Astronomy

1

M29(=Ngc 6913), Open Cluster, Variable, Photometry

Scientific paper

We present results of time-series CCD photometry for 178 stars in the young open cluster M29(=NGC6913). Total 1036 V-band CCD frames were collected for five nights between August 12 and September 13, 1994. The photometric precision is about 7.6mmag for 9th-10th mag stars in M29 with exposure times of 30 seconds. From the dispersion diagram and the light curves, one detached eclipsing binary(HD194378) and two suspected variables are newly discovered. A gamma Cas type variable, V1322 Cyg, which has been known as a member of M29, did not show any light variations during the period of present observations, indicating that it passed the steady phase withough the eruption during our observing runs.

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