Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations
We explored the role of X-ray binaries composed by a black hole and a massive stellar companion [black hole X-ray binaries (BHXs)] as sources of kinetic feedback by using hydrodynamical cosmological simulations. Following previous results, our BHX model selects metal-poor stars (Z = [0, 10-4]) as po...
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Autores principales: | Artale, M.C., Tissera, P.B., Pellizza, L.J. |
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Formato: | JOUR |
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v448_n4_p3071_Artale |
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