Wideband Photometry of the Eclipsing Binary Star 68 Herculis

Details Wideband Photometry of the Eclipsing Binary Star 68 Herculis Wideband Photometry of the Eclipsing Binary Star 68 Herculis

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aps..tss..ce10m&link_type=abstract

American Physical Society, Texas Section Spring Meeting, March 15-16, 1996, abstract #CE.10

Physics

Scientific paper

68 Herculis, a Beta Lyra type eclipsing binary star, is being studied by an undergraduate and a graduate student at Texas A&M University, using the University's 14-inch Schmidt-Cassegrain telescope and an Optec SSP-3 Photometer. The star's orbital period and epoch are being determined in order to see if the system has evolved since these were last measured.

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