RX J0719.2+6557: A New Eclipsing Polar

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dc.creatorTovmassian, G.
dc.creatorGreiner, J.
dc.creatorZickgraf, F. -J.
dc.creatorKroll, P.
dc.creatorKrautter, J.
dc.creatorThiering, I.
dc.creatorSerrano, A.
dc.date1996-09-24
dc.date.accessioned2026-07-07T02:21:57Z
dc.date.available2026-07-07T02:21:57Z
dc.descriptionA 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.
dc.descriptionto appear in "Accretion Phenomena and Associated Outflows", IAU Coll. 163, Port Douglas, Australia, July 1996; 2 pages LATEX with paspconf style file, including 1 ps-figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9609166
dc.identifierhttp://arxiv.org/abs/astro-ph/9609166
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10700
dc.subjectAstrophysics
dc.titleRX J0719.2+6557: A New Eclipsing Polar
dc.typetext

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