Post common envelope binaries from the SDSS

Free access article

Issue		A&A Volume 500, Number 2, June III 2009


Page(s)		867 - 872
Section		Stellar structure and evolution
DOI		http://dx.doi.org/10.1051/0004-6361/200911699
Published online		29 April 2009

A&A 500, 867-872 (2009)
DOI: 10.1051/0004-6361/200911699

VI. SDSS J120615.73+510047.0: a new low accretion rate magnetic binary

A. D. Schwope¹, A. Nebot Gomez-Moran¹, M. R. Schreiber², and B. T. Gänsicke³

¹ Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
e-mail: aschwope@aip.de
² Departamento de Física y Astronomía, Universidad de Valparaíso, Avenida Gran Bretana 1111, Valparaíso, Chile
³ Department of Physics, University of Warwick, Coventry CV4 7AL, UK

Received 22 January 2009 / Accepted 18 March 2009

Abstract
We report the discovery of the ninth pre-polar consisting of a late-type ZAMS secondary and a magnetic white dwarf. The white dwarf accretes at an extreme low rate, $\dot{M} \sim 10^{-14}$ $M_\odot$ yr^-1, from the wind of the companion donor star. The source was found in our systematic search for WD/MS binaries within SDSS/SEGUE. Based on seven Sloan spectra we estimate a binary period of ~200, 230, or 270 min. The UV to IR spectral energy distribution was decomposed into a dM3-dM4 ZAMS secondary and a cool white dwarf, ~9000 K, which consistently imply a distance between 360 and 420 pc. The optical spectrum displays one pronounced cyclotron hump, likely originating from a low-temperature plasma, ~1 keV, in a field of 108 MG. We comment on the evolutionary link between polars and pre-polars.

Key words: accretion, accretion disks -- stars: magnetic fields -- binaries: close -- stars: individual: SDSS J120615.73+510047.0

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