2XMMiJ225036.9+573154 - a new eclipsing AMHer binary discovered using XMM-Newton
Abstract
We report the discovery of an eclipsing polar, 2XMMiJ225036.9+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 174min. An extended pre-eclipse absorption dip is observed in soft X-rays at φ = 0.8-0.9, with evidence for a further dip in the soft X-ray light curve at φ ~ 0.4. Further, X-rays are seen from all orbital phases (apart from the eclipse) which make it unusual amongst eclipsing polars. We have identified the optical counterpart, which is faint (r = 21), and shows a deep eclipse (>3.5mag 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 Hα in emission for a fraction of the orbital period.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- May 2009
- DOI:
- 10.1111/j.1365-2966.2009.14528.x
- arXiv:
- arXiv:0901.3095
- Bibcode:
- 2009MNRAS.395..416R
- Keywords:
-
- binaries: close;
- stars: individual: 2XMMiJ225036.9+573154;
- novae;
- cataclysmic variables;
- X-rays: binaries;
- Astrophysics - Galaxy Astrophysics;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- Accepted for publication in MNRAS