RX J1313.2-3259, a long-period Polar discovered with ROSAT
Astronomy & Astrophysics
in press
Contact: aschwope@aip.de
Preprint of paper
H.-C. Thomas [1], K. Beuermann [2], V. Burwitz [3], K. Reinsch [2], A.D. Schwope [4]
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Max-Planck-Institut f¨r Astrophysik,
Karl-Schwarzschild-Strasse 1, D-85748 Garching, Germany
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Universitätssternwarte Göttingen, Geismarlandstrasse 11,
D--37083 Göttingen, Germany
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Max-Planck-Institut f¨r Extraterrestrische Physik,
Karl-Schwarzschild-Strasse 1, D-85748 Garching, Germany
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Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam,
Germany
Abstract:
We report observations of a new AM Herculis binary identified
as the optical counterpart of the X-ray source RX J1313.2-3259,
detected during the ROSAT All-Sky Survey (RASS). It has an orbital period
of 251 min and is strongly modulated at optical wavelengths. The
long-term behavior is characterized by a pronounced variation in X-rays
between the RASS and two subsequent pointings (decrease
by a factor 40 in count rate) and by moderate changes in the optical brightness (up to a
factor 5). The X-ray spectrum is dominated by a soft quasi-blackbody component,
with a smaller contribution from thermal bremsstrahlung. Measurements of
high circular polarization confirm its classification as a Polar with a
magnetic field strength of 56 MG. The average visual magnitude of RX J1313.2-3259 is
V = 16m, for its distance we get 200 pc.