Time Series Photometry Of The High Mass X-ray Binary LPH 128 And The δ Scuti Star GSC 03973-01698

Details Time Series Photometry Of The High Mass X-ray Binary LPH 128 And The δ Scuti Star GSC 03973-01698 Time Series Photometry Of The High Mass X-ray Binary LPH 128 And The δ Scuti Star GSC 03973-01698

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21343304b&link_type=abstract

American Astronomical Society, AAS Meeting #213, #433.04; Bulletin of the American Astronomical Society, Vol. 41, p.301

Astronomy and Astrophysics

Astronomy

Scientific paper

As part of our ongoing variable star program, and a summer REU program, we observed the field around the High Mass X-ray Binary system LPH 128. We obtained 19 nights of photometry between 13 June, 2008 and 9 August, 2008 using the 0.4-m David Derrick Telescope at our campus observatory and the 0.4-m and 0.5-m telescopes of the West Mountain Observatory. We will present the results of our observations of LPH 128 and the delta Scuti star GSC 03973-01698 that is in the same field of view. For GSC 03973-01698 we found a new period of 0.065073 days.
This work was conducted as part of a summer Research Experience for Undergraduates program held at BYU. We would like to acknowledge NSF grant PHY-0552795.

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