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Abstract:

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 possible progenitors. The model that better reproduces observations assumes that an ~20 per cent fraction of low-metallicity black holes are in binary systems which produces BHXs. These sources are estimated to deposit ~1052 erg of kinetic energy per event. With these parameters and in the simulated volume, we find that the energy injected by BHXs represents ~30 per cent of the total energy released by Type II supernova and BHX events at redshift z ~ 7 and then decreases rapidly as baryons get chemically enriched. Haloes with virial masses smaller than ~1010M{bull's eye} (or Tvir ≤105 K) are the most directly affected ones by BHX feedback. These haloes host galaxies with stellar masses in the range 107-108 M{bull's eye}. Our results show that BHX feedback is able to keep the interstellar medium warm, without removing a significant gas fraction, in agreement with previous analytical calculations. Consequently, the stellar-to-dark matter mass ratio is better reproduced at high redshift. Our model also predicts a stronger evolution of the number of galaxies as a function of the stellar mass with redshift when BHX feedback is considered. These findings support previous claims that the BHXs could be an effective source of feedback in early stages of galaxy evolution. © 2015 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society.

Registro:

Documento: Artículo
Título:Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations
Autor:Artale, M.C.; Tissera, P.B.; Pellizza, L.J.
Filiación:Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), C.C. 67 Suc. 28, Ciudad de Buenos Aires, C1428ZAA, Argentina
Departamento de Ciencias Fisicas, Universidad Andres Bello, Av. Republica 220, Santiago, 8370134, Chile
Millennium Institute of Astrophysics, Av. Republica 220, Santiago, 8370134, Chile
Instituto Argentino de Radioastronomía, CONICET, C. C. 5 (1894), Villa Elisa, Prov. de, Buenos Aires, Argentina
Palabras clave:Abundances - galaxies; Binaries; Evolution - galaxies; Galaxies; High-redshift -X-rays
Año:2015
Volumen:448
Número:4
Página de inicio:3071
Página de fin:3080
DOI: http://dx.doi.org/10.1093/mnras/stv218
Título revista:Monthly Notices of the Royal Astronomical Society
Título revista abreviado:Mon. Not. R. Astron. Soc.
ISSN:00358711
CODEN:MNRAA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v448_n4_p3071_Artale

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Citas:

---------- APA ----------
Artale, M.C., Tissera, P.B. & Pellizza, L.J. (2015) . Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations. Monthly Notices of the Royal Astronomical Society, 448(4), 3071-3080.
http://dx.doi.org/10.1093/mnras/stv218
---------- CHICAGO ----------
Artale, M.C., Tissera, P.B., Pellizza, L.J. "Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations" . Monthly Notices of the Royal Astronomical Society 448, no. 4 (2015) : 3071-3080.
http://dx.doi.org/10.1093/mnras/stv218
---------- MLA ----------
Artale, M.C., Tissera, P.B., Pellizza, L.J. "Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations" . Monthly Notices of the Royal Astronomical Society, vol. 448, no. 4, 2015, pp. 3071-3080.
http://dx.doi.org/10.1093/mnras/stv218
---------- VANCOUVER ----------
Artale, M.C., Tissera, P.B., Pellizza, L.J. Stellar feedback from high-mass X-ray binaries in cosmological hydrodynamical simulations. Mon. Not. R. Astron. Soc. 2015;448(4):3071-3080.
http://dx.doi.org/10.1093/mnras/stv218