New Observations of AC Ursa Majoris

Details New Observations of AC Ursa Majoris New Observations of AC Ursa Majoris

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.6019m&link_type=abstract

American Astronomical Society, AAS Meeting #211, #60.19; Bulletin of the American Astronomical Society, Vol. 39, p.846

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present light curves and analysis of the eclipsing variable star AC Ursa Majoris. AC UMa is a detached Algol-type eclipsing system. It's eclipse depth and period have been reported in the literature, but vary significantly in reported values from roughly 1 magnitude to 4 magnitudes. This effort, using a 44cm Newtonian telescope and CCD camera of the Center for Backyard Astrophysics and historical data from other telescopes, attempts to rectify the discrepancies in the literature and present new timings of the maximum and minimum eclipses and their depths in preparation for a more detailed study of this interesting system.

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