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Wevers (Radboud U.)","submitted_at":"2016-12-06T00:58:52Z","abstract_excerpt":"We present the results of a photometric and spectroscopic analysis of the Galactic Bulge Survey X-ray source CXOGBS J174954.5-294335 (hereafter, referred to as CX19). CX19 is a long period, eclipsing intermediate polar type cataclysmic variable with broad, single-peaked Balmer and Paschen emission lines along with HeII $\\lambda4686$ and Bowen blend emission features. With coverage of one full and two partial eclipses and archival photometry, we determine the ephemeris for CX19 to be HJD(eclipse) = 2455691.8581(5) + 0.358704(2)$\\times$N. 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Heinke (U. Alberta), Christopher B. Johnson (LSU, C. T. Britt (MSU, D. Steeghs (Warwick), Jianfeng Wu (UofM), M. A. P. Torres (SRON, P. G. Jonker (SRON, Radboud U.), R. I. Hynes (LSU), STScI), T. Maccarone (TTU), TTU), T. Wevers (Radboud U.)","submitted_at":"2016-12-06T00:58:52Z","abstract_excerpt":"We present the results of a photometric and spectroscopic analysis of the Galactic Bulge Survey X-ray source CXOGBS J174954.5-294335 (hereafter, referred to as CX19). CX19 is a long period, eclipsing intermediate polar type cataclysmic variable with broad, single-peaked Balmer and Paschen emission lines along with HeII $\\lambda4686$ and Bowen blend emission features. With coverage of one full and two partial eclipses and archival photometry, we determine the ephemeris for CX19 to be HJD(eclipse) = 2455691.8581(5) + 0.358704(2)$\\times$N. 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