The High Mass X-ray binaries in star-forming galaxies
作者： M. Celeste Artale , Nicola Giacobbo , Michela Mapelli , Paolo Esposito
DOI: 10.1017/S1743921318007627
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摘要: The high mass X-ray binaries (HMXBs) provide an exciting framework to investigate the evolution of massive stars and processes behind binary evolution. HMXBs have shown be good tracers recent star formation in galaxies might important feedback sources at early stages Universe. Furthermore, are likely progenitors gravitational wave (BH–BH or BH–NS that may merge producing waves). In this work, we nature properties HMXB population star-forming galaxies. We combine results from synthesis model MOBSE (Giacobbo & Mapelli 2018a) together with galaxy catalogs EAGLE simulation (Schaye et al. 2015). Therefore, method describes within their host a self-consistent way. compute luminosity function (XLF) galaxies, showing methodology matches main features observed XLF.
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