@conference {23888,
	title = {Small Magellanic Cloud: Star-Formation History and X-Ray Binary Populations},
	volume = {424},
	year = {2010},
	month = {2010/07/1},
	pages = {230},
	abstract = {Using Chandra, XMM-Newton and optical photometric catalogs we study the young XRB populations of the SMC. We find that the Be-XRBs are observed in regions with star formation (SF) 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 SF (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 10<SUP>-6</SUP> M<SUB>sun</SUB>/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.},
	isbn = {1050-3390},
	url = {https://ui.adsabs.harvard.edu/abs/2010ASPC..424..230A},
	author = {Antoniou, V. and Zezas, A. and Hatzidimitriou, D. and Kalogera, V.}
}
