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Two Rare Magnetic Cataclysmic Variables with Extreme Cyclotron Features Identified in the Sloan Digital Sky Survey

Paula Szkody·Scott F. Anderson·Gary Schmidt·Patrick B. Hall·Bruce Margon·Antonino Miceli·Mark SubbaRao·James Frith·Hugh Harris
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Abstract

Two newly identified magnetic cataclysmic variables discovered in the Sloan Digital Sky Survey (SDSS), SDSSJ155331.12+551614.5 and SDSSJ132411.57+032050.5, have spectra showing highly prominent, narrow, strongly polarized cyclotron humps with amplitudes that vary on orbital periods of 4.39 and 2.6 hrs, respectively. In the former, the spacing of the humps indicates the 3rd and 4th harmonics in a magnetic field of ~60 MG. The narrowness of the cyclotron features and the lack of strong emission lines imply very low temperature plasmas and very low accretion rates, so that the accreting area is heated by particle collisions rather than accretion shocks. The detection of rare systems like these exemplifies the ability of the SDSS to find the lowest accretion rate close binaries.

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Paula Szkody, Scott F. Anderson, Gary Schmidt, Patrick B. Hall, Bruce Margon, Antonino Miceli, Mark SubbaRao, James Frith, Hugh Harris. 2002-10-11. Two Rare Magnetic Cataclysmic Variables with Extreme Cyclotron Features Identified in the Sloan Digital Sky Survey. https://doi.org/10.1086/345418

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