Astronomy and Astrophysics
We report the discovery of a new cataclysmic binary star from the ROSAT Galactic Plane Survey. The star has V >∼ 18.5atminimumlightandwehavemeasureditasbrightasV = 15.7. Spectroscopy shows broad hydrogen and helium emission lines; HeII λ4686 is not detected. Hα radial velocities yield an orbital period of 0.1429 ± 0.0004 d (3.430 ± 0.010 h). Time- series photometry covering one orbital cycle near maximum light shows irregular variability, but no evidence of an eclipse. ThesystemappearstobeanewdwarfnovaoftheUGemorZ Cam type, and is unlikely to be a magnetic system. Its period is unusually short for a U Gem star.
Curiously, the new cataclysmic binary is 83′′ from the orig- inal ROSAT PSPC survey position, which puts it outside the PSPC positional uncertainty. Follow-up observations with the HRI reveal that the PSPC source is the superposition of two sources, and the cataclysmic is much the weaker of the two in X-rays. Its discovery in this survey is therefore essentially acci- dental. A V = 19.4 mag star is located 1.2′′ from the stronger source’s HRI position.
Thorstensen, J R. and F Haberl, "A Newly-Discovered Cataclysmic Binary Near the ROSAT Galactic Plane Source RX J1910.8+2856" (2000). Open Dartmouth: Peer-reviewed articles by Dartmouth faculty. 539.