http://arxiv.org/abs/1906.07767
We report the discovery of a new eclipsing polar, CRTS J035010.7+323230 (hereafter CRTS J0350+3232). We identified this cataclysmic variable (CV) candidate as a possible polar from its multi-year Catalina Real-Time Transient Survey (CRTS) optical light curve. Photometric monitoring of 22 eclipses in 2015 and 2017 was performed with the 2.1-m Otto Struve Telescope at McDonald Observatory. We derive an unambiguous high-precision ephemeris. Strong evidence that CRTS J0350+3232 is a polar comes from optical spectroscopy obtained over a complete orbital cycle using the Apache Point Observatory 3.5-m telescope. High velocity Balmer and He II $\lambda$4686{\AA} emission line equivalent width ratios, structures, and variations are typical of polars and are modulated at the same period, 2.37-hrs (142.3-min), as the eclipse to within uncertainties. The spectral energy distribution and luminosity is found to be comparable to that of AM Herculis. Pre-eclipse dips in the light curve show evidence for stream accretion. We derive the following tentative binary and stellar parameters assuming a helium composition white dwarf and a companion mass of 0.2 M${\odot}$: inclination i = 74.68$^{o}$ ${\pm}$ 0.03$^{o}$, semi-major axis a = 0.942 ${\pm}$ 0.024 R${\odot}$, and masses and radii of the white dwarf and companion respectively: M${1}$ = 0.948 $^{+0.006}{-0.012}$ M${\odot}$, R${1}$ = 0.00830 $^{+0.00012}{-0.00006}$ R${\odot}$, R${2}$ = 0.249 ${\pm}$ 0.002 R${\odot}$. As a relatively bright (V $\sim$ 17-19 mag), eclipsing, period-gap polar, CRTS J0350+3232 will remain an important laboratory for the study of accretion and angular momentum evolution in polars.
P. Mason, N. Wells, M. Motsoaledi, et. al.
Thu, 20 Jun 19
16/51
Comments: 11 pages, 15 figures
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