{ "id": "0901.3095", "version": "v1", "published": "2009-01-20T16:41:43.000Z", "updated": "2009-01-20T16:41:43.000Z", "title": "2XMMi J225036.9+573154 - a new eclipsing AM Her binary discovered using XMM-Newton", "authors": [ "Gavin Ramsay", "Simon Rosen", "Pasi Hakala", "Thomas Barclay" ], "comment": "Accepted for publication in MNRAS", "doi": "10.1111/j.1365-2966.2009.14528.x", "categories": [ "astro-ph.GA", "astro-ph.HE" ], "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.", "revisions": [ { "version": "v1", "updated": "2009-01-20T16:41:43.000Z" } ], "analyses": { "keywords": [ "xmm-newton", "distinct soft x-ray component", "soft x-ray light curve", "eclipsing polar", "extended pre-eclipse absorption dip" ], "tags": [ "journal article" ], "publication": { "publisher": "Wiley-Blackwell", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2009, "month": "May", "volume": 395, "number": 1, "pages": 416 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 811588, "adsabs": "2009MNRAS.395..416R" } } }