A Bright Stellar Variability Survey in the NGC 6811 Region

Details A Bright Stellar Variability Survey in the NGC 6811 Region A Bright Stellar Variability Survey in the NGC 6811 Region

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20916207h&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #162.07; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present preliminary results of a BVRI variability survey conducted by the AAVSO in coordination with the BOKS program during the month of September. Stars in a 1.5x0.75 degree field centered on the open cluster NGC 6811 in Cygnus were monitored. Many new variables brighter than V=15 were discovered, and light curves of several existing or suspected variables in the region were created. A description of the observing program, highlights from some of the more prolific amateur contributors, and lightcurves of the variables will be presented.

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