Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.0412m&link_type=abstract
American Astronomical Society, 191st AAS Meeting, #04.12; Bulletin of the American Astronomical Society, Vol. 29, p.1212
Astronomy and Astrophysics
Astronomy
Scientific paper
Under the sponsorship of the NSF, a multi-year program has been established at New Mexico State University to have undergraduate students monitor different classes of variable stars. Amongst our targets are the optical counterparts of high-energy sources such as Low-Mass X-ray Binaries (LMXBs), Algol eclipsing binaries, and cataclysmic variables. This program included the installation, and debugging of a 16" Meade telescope at the NMSU campus observatory. This telescope is equipped with a Santa Barbara Instruments Group ST-8 CCD camera, and a standard UBVRI filter set. The students are responsible for collecting the data, reducing the CCD images, and modeling their results. During the Fall semester we have a program of monitoring infrequently observed Algol eclipsing binaries. Our students will determine the system parameters of these Algol binaries by modeling the photometry they have obtained using a light curve synthesis program (``Binary Maker 2.0'', by D. Bradstreet). [For the initial results of this program see the poster by P. A. Mason et al.] During the Spring semester we anticipate an intense monitoring program of the LMXB Sco X-1. The optical data will be combined with simultaneous 10-20 keV data from the BATSE Spectroscopy Detectors on the Compton Gamma-Ray Observatory to understand how the x-rays are reprocessed in the accretion disk surrounding the neutron star in Sco X-1.
French Marcus
Galvan Javier
Harrison Thomas E.
Jarvis Thomas
Mason Paul A.
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