{ "id": "1006.2381", "version": "v1", "published": "2010-06-11T20:00:03.000Z", "updated": "2010-06-11T20:00:03.000Z", "title": "Star formation history and X-ray binary populations: the case of the Small Magellanic Cloud", "authors": [ "Vallia Antoniou", "Andreas Zezas", "Despina Hatzidimitriou", "Vicky Kalogera" ], "comment": "15 pages, 2 figures, published in ApJ Letters", "journal": "ApJ 716L.140A 2010", "categories": [ "astro-ph.HE" ], "abstract": "Using Chandra, XMM-Newton, and optical photometric catalogs we study the young X-ray binary (XRB) populations of the Small Magellanic Cloud. We find that the Be/X-ray binaries (Be-XRBs) are observed in regions with star formation rate bursts ~25-60 Myr ago. The similarity of this age with the age of maximum occurrence of the Be phenomenon (~40 Myr) indicates that the presence of a circumstellar decretion disk plays a significant role in the number of observed XRBs in the 10-100 Myr age range. We also find that regions with strong but more recent star formation (e.g., the Wing) are deficient in Be-XRBs. By correlating the number of observed Be-XRBs with the formation rate of their parent populations, we measure a Be-XRB production rate of ~1 system per 3 x 10^(-3) M$_{\\odot}$/yr. Finally, we use the strong localization of the Be-XRB systems in order to set limits on the kicks imparted on the neutron star during the supernova explosion.", "revisions": [ { "version": "v1", "updated": "2010-06-11T20:00:03.000Z" } ], "analyses": { "keywords": [ "small magellanic cloud", "x-ray binary populations", "star formation history", "circumstellar decretion disk plays", "star formation rate bursts" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/716/2/L140", "journal": "The Astrophysical Journal", "year": 2010, "month": "Jun", "volume": 716, "number": 2 }, "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable", "inspire": 858176, "adsabs": "2010ApJ...716L.140A" } } }