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RX J0719.2+6557: A New Eclipsing Polar

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arxiv astro-ph/9609166 v1 submitted 1996-09-24 astro-ph

G. Tovmassian (UNAM , Mexico) , J. Greiner , F.-J. Zickgraf (Garching , Germany) , P. Kroll (Sonneberg , J. Krautter , I. Thiering (Heidelberg
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A. Serrano (INAOE
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classification astro-ph
keywords eclipsingemissionheatedj0719secondarysourcestrongaccretion
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A new magnetic, eclipsing cataclysmic variable is identified as the counterpart of the X-ray source RX J0719.2+6557 detected during the ROSAT all-sky survey. The relative phasing of photometric and spectroscopic periods indicates a self-eclipsing system. Doppler tomography points to the heated surface of the secondary as a strong source of emission and of diskless accretion. Near-infrared spectroscopy revealed two unusual strong emission features originating on the heated side of the secondary.

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Cited by 1 Pith paper

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  1. MASTER OT J072007.30+451611.6: A Polar with Strong Optical Variability and Suppressed He II Emission

    astro-ph.SR 2025-07 conditional novelty 5.0 of 10

    J0720 is confirmed as a magnetic cataclysmic variable (polar) with a 1.5-hour orbit, stream-fed accretion without a disk, and unusually weak He II emission relative to H beta.

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