2XMMi J225036.9+573154 - a new eclipsing AM Her binary discovered using XMM-Newton
Abstract
We report the discovery of an eclipsing polar, 2XMMi J225036.9+573154, using XMM-Newton. It was discovered by searching the light curves in the 2XMMi catalogue for objects showing X-ray variability. Its X-ray light curve shows a total eclipse of the white dwarf by the secondary star every 174 mins. An extended pre-eclipse absorption dip is observed in soft X-rays at phi=0.8-0.9, with evidence for a further dip in the soft X-ray light curve at phi~0.4. Further, X-rays are seen from all orbital phases (apart from the eclipse) which makes it unusual amongst eclipsing polars. We have identified the optical counterpart, which is faint (r=21), and shows a deep eclipse (>3.5 mag in white light). Its X-ray spectrum does not show a distinct soft X-ray component which is seen in many, but not all, polars. Its optical spectrum shows Halpha in emission for a fraction of the orbital period.
Keywords
Cite
@article{arxiv.0901.3095,
title = {2XMMi J225036.9+573154 - a new eclipsing AM Her binary discovered using XMM-Newton},
author = {Gavin Ramsay and Simon Rosen and Pasi Hakala and Thomas Barclay},
journal= {arXiv preprint arXiv:0901.3095},
year = {2009}
}
Comments
Accepted for publication in MNRAS