Monthly Notices of the Royal Astronomical Society
Department of Physics and Astronomy
We present spectroscopy and orbital periods Porb of four relatively little-studied cataclysmic variable stars. The stars and their periods are: AF Cam, Porb = 0.324(1) d (the daily cycle count is slightly ambiguous); V2069 Cyg (= RX J2123.7+4217), 0.311683(2) d; PG 0935+075, 0.1868(3) d; and KUV 03580+0614, 0.1495(6) d. V2069 Cyg and KUV 03580+0614 both show He iiλ4686 emission comparable in strength to Hβ. V2069 Cyg appears to be a luminous nova-like variable, and the strong He ii suggests it may be an intermediate polar. The period of KUV 03580+0614 is similar to members of the SW Sex-type nova-like variables, and it shows the phase-dependent absorption in the Balmer and He i lines typical of this subclass. AF Cam shows absorption features from a K-type secondary, as expected given its rather long orbital period. The secondary spectrum and the outburst magnitude both suggest that AF Cam is approximately 1 kpc distant. The spectrum of PG 0935+075 resembles that of a dwarf nova at minimum light, with a noticeable contribution from an M-dwarf secondary star. The secondary spectrum and a tentative outburst magnitude both suggest a distance near 500 pc.
John R. Thorstensen, Cynthia J. Taylor, Spectroscopy and orbital periods of four cataclysmic variable stars, Monthly Notices of the Royal Astronomical Society, Volume 326, Issue 4, October 2001, Pages 1235–1242, https://doi.org/10.1111/j.1365-2966.2001.04680.x
Dartmouth Digital Commons Citation
Thorstensen, John R. and Taylor, Cynthia J., "Spectroscopy and Orbital Periods of Four Cataclysmic Variable Stars" (2001). Dartmouth Scholarship. 1868.