Photometric Monitoring of the PMS Object Walker 90

Details Photometric Monitoring of the PMS Object Walker 90 Photometric Monitoring of the PMS Object Walker 90

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.3015j&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #30.15; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

It has long been known that the interesting pre-main sequence object Walker 90 (V590 Mon) located in the young open cluster NGC 2264 displays photometric variability on many time scales. We present BVRI and H-alpha photometry from a variety of epochs in order to better understand the nature and scale of these variations. The majority of the observations were secured using the 0.8-m telescope at the Tenagra robotic observatory in southern Arizona during the past four observing seasons.
We acknowledge partial support for this work from the AAS in the form of a Small Research Grant. We also thank the Department of Physics and Astronomy at Brigham Young University for continued support of this research.

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