Two new magnetic cataclysmic variables discovered in the 3XMM catalogue

Context. X-ray catalogues provide a wealth of information on many source types, ranging from compact objects to galaxies, clusters of galaxies, stars, and even planets. Thanks to the huge volume of X-ray sources provided in the 3XMM catalogue, along with many source specific products, many new examp...

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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 2018, Vol.615, p.A133
Main Authors: Webb, N. A., Schwope, A., Zolotukhin, I., Lin, D., Rosen, S. R.
Format: Article
Language:English
Subjects:
accretion
accretion disks
Astrophysics
Cataclysmic variables
Compact galaxies
Galaxies
novae
Orbits
Photometry
Physics
Quality control
Sky surveys (astronomy)
White dwarf stars
white dwarfs
X ray sources
X ray spectra
X-rays: individuals: 3XMM J183333.1+225136
X-rays: individuals: 3XMM J184916.1+652943
XMM (spacecraft)
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Summary:Context. X-ray catalogues provide a wealth of information on many source types, ranging from compact objects to galaxies, clusters of galaxies, stars, and even planets. Thanks to the huge volume of X-ray sources provided in the 3XMM catalogue, along with many source specific products, many new examples from rare classes of sources can be identified. Aims. Through visualising spectra and lightcurves from about 80 observations included in the incremental part of the 3XMM catalogue, 3XMM-DR5, as part of the quality control of the catalogue, we identified two new X-ray sources, 3XMM J183333.1+225136 and 3XMM J184916.1+652943, that were highly variable. This work aims to investigate their nature. Methods. Through simple model fitting of the X-ray spectra and analysis of the X-ray lightcurves of 3XMM J183333.1+225136 and 3XMM J184916.1+652943, along with complementary photometry from the XMM-Newton Optical Monitor, Pan-STARRS and the Stella/WiFSIP and Large Binocular Telescope (LBT) spectra, we suggest that the two sources might be magnetic cataclysmic variables (CVs) of the polar type and we determine some of their properties. Results. Both CVs have very hard spectra, showing no soft excess. They are both situated in the local neighbourhood, located within ~1 kpc. 3XMM J183333.1+225136 has an orbital period of 2.15 h. It shows features in the lightcurve that may be a total eclipse of the white dwarf. 3XMM J184916.1+652943 has an orbital period of 1.6 h. Given that only a small sky area was searched to identify these CVs, future sensitive all sky surveys such as the eROSITA project should be very successful at uncovering large numbers of such sources.
ISSN:0004-6361
1432-0746
1432-0756
DOI:10.1051/0004-6361/201730974