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Chisari, N.E.; Tissera, P.B.; Pellizza, L.J. "Host galaxies of long gamma-ray bursts in the Millennium Simulation" (2010) Monthly Notices of the Royal Astronomical Society. 408(1):647-656
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Abstract:

In this work, we investigate the nature of the host galaxies of long gamma-ray bursts (LGRBs) using a galaxy catalogue constructed from the Millennium Simulation. We developed an LGRB synthetic model based on the hypothesis that these events originate at the end of the life of massive stars following the collapsar model, with the possibility of including a constraint on the metallicity of the progenitor star. A complete observability pipeline was designed to calculate a probability estimation for a galaxy to be observationally identified as a host for LGRBs detected by present observational facilities. This new tool allows us to build an observable host galaxy catalogue which is required to reproduce the current stellar mass distribution of observed hosts. This observability pipeline predicts that the minimum mass for the progenitor stars should be ~ 75 M. in order to be able to reproduce BATSE observations. Systems in our observable catalogue are able to reproduce the observed properties of host galaxies, namely stellar masses, colours, luminosity, star formation activity and metallicities as a function of redshift. At z > 2, our model predicts that the observable host galaxies would be very similar to the global galaxy population. We found that ~ 88 per cent of the observable host galaxies with mean gas metallicity lower than 0.6 Z. have stellar masses in the range 108.5-1010.3 M., in excellent agreement with observations. Interestingly in our model, observable host galaxies remain mainly within this mass range regardless of redshift, since lower stellar mass systems would have a low probability of being observed while more massive ones would be too metal-rich. Observable host galaxies are predicted to preferentially inhabit dark matter haloes in the range 1011-1011.5 M., with a weak dependence on redshift. They are also found to preferentially map different density environments at different stages of evolution of the Universe. At high redshifts, the observable host galaxies are predicted to be located in similar environments as the global galaxy population but have a slightly higher probability to have a close companion. © 2010 The Authors. Journal compilation © 2010 RAS.

Registro:

Documento: Artículo
Título:Host galaxies of long gamma-ray bursts in the Millennium Simulation
Autor:Chisari, N.E.; Tissera, P.B.; Pellizza, L.J.
Filiación:Instituto de Astronomía y Física del Espacio, Casilla de Correo 67, Suc. 28, 1428, Buenos Aires, Argentina
Consejo Nacional de Investigaciones Científicas y Técnicas, CONICET, Argentina
Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, United States
Palabras clave:Galaxies: evolution; Galaxies: interactions; Galaxies: star formation; Gamma-rays: bursts
Año:2010
Volumen:408
Número:1
Página de inicio:647
Página de fin:656
DOI: http://dx.doi.org/10.1111/j.1365-2966.2010.17169.x
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_v408_n1_p647_Chisari

Referencias:

  • Bell, E.F., McIntosh, D.H., Katz, N., Weinberg, M.D., (2003) ApJS, 149, p. 289
  • Bissaldi, E., Calura, F., Matteucci, F., Longo, F., Barbiellini, G., (2007) A&A, 471, p. 585
  • Bloom, J.S., Djorgovski, S.G., Kulkarni, S.R., (2001) ApJ, 554, p. 678
  • Bloom, J.S., Berger, E., Kulkarni, S.R., Djorgovski, S.G., Frail, D.A., (2003) AJ, 125, p. 999
  • Bornancini, C.G., Martínez, H.J., Lambas, D.G., Le Floc'h, E., Mirabel, I.F., Minniti, D., (2004) ApJ, 614, p. 84
  • Campisi, M.A., De Lucia, G., Li, L.X., Mao, S., Kang, X., (2009) MNRAS, 400, p. 1613
  • Castro Cerón, J.M., Michalowski, M.J., Hjorth, J., Malesani, D., Gorosabel, J., Watson, D., Fynbo, J.P.U., (2008), (arXiv:0803.2235); Chabrier, G., (2003) PASP, 115, p. 763
  • Christensen, L., Hjorth, J., Gorosabel, J., (2004) A&A, 425, p. 913
  • Cole, S., (1991) ApJ, 367, p. 45
  • Courty, S., Björnsson, G., Gudmundsson, E.H., (2004) MNRAS, 354, p. 581
  • Daigne, F., Rossi, E.M., Mochkovitch, R., (2006) MNRAS, 372, p. 1034
  • De Lucia, G., Blaizot, J., (2007) MNRAS, 375, p. 2
  • De Rossi, M.E., Tissera, P.B., De Lucia, G., Kauffmann, G., (2009) MNRAS, 395, p. 210
  • Di Matteo, P., Bournaud, F., Martig, M., Combes, F., Melchior, A.L., Semelin, B., (2008) A&A, 492, p. 31
  • Frail, D.A., (2001) ApJ, 562, pp. L55
  • Frontera, F., (2009) ApJS, 180, p. 192
  • Fryer, C.L., Woosley, S.E., Hartmann, D.H., (1999) ApJ, 526, p. 152
  • Fynbo, J.P.U., (2002) A&A, 388, p. 425
  • Fynbo, J.P.U., (2009) ApJS, 185, p. 526
  • Galama, T.J., (1998) Nat, 395, p. 670
  • Glazebrook, K., (2004) Nat, 430, p. 181
  • Guetta, D., Piran, T., (2007) J. Cosmology Astropart. Phys., 7, p. 3
  • Hirschi, R., Meynet, G., Maeder, A., (2005) A&A, 443, p. 581
  • Hjorth, J., (2003) Nat, 423, p. 847
  • Hurley, K., (1992) A&AS, 92, p. 401
  • Jakobsson, P., (2005) MNRAS, 362, p. 245
  • Katz, N., Gunn, J.E., (1991) ApJ, 377, p. 365
  • Kauffmann, G., White, S.D.M., Heckman, T.M., Ménard, B., Brinchmann, J., Charlot, S., Tremonti, C., Brinkmann, J., (2004) MNRAS, 353, p. 713
  • Kouveliotou, C., Meegan, C.A., Fishman, G.J., Bhat, N.P., Briggs, M.S., Koshut, T.M., Paciesas, W.S., Pendleton, G.N., (1993) ApJ, 413, pp. L101
  • Lacey, C., Silk, J., (1991) ApJ, 381, p. 14
  • Lambas, D.G., Tissera, P.B., Alonso, M.S., Coldwell, G., (2003) MNRAS, 346, p. 1189
  • Le Floc'h, E., (2003) A&A, 400, p. 499
  • MacFadyen, A.I., Woosley, S.E., (1999) ApJ, 524, p. 262
  • Mészáros, P., (2006) Rep. Progress Phys., 69, p. 2259
  • Metzger, M.R., Djorgovski, S.G., Kulkarni, S.R., Steidel, C.C., Adelberger, K.L., Frail, D.A., Costa, E., Frontera, F., (1997) Nat, 387, p. 878
  • Modjaz, M., (2008) AJ, 135, p. 1136
  • Mosconi, M.B., Tissera, P.B., Lambas, D.G., Cora, S.A., (2001) MNRAS, 325, p. 34
  • Navarro, J.F., White, S.D.M., (1993) MNRAS, 265, p. 271
  • Nuza, S.E., Tissera, P.B., Pellizza, L.J., Lambas, D.G., Scannapieco, C., De Rossi, M.E., (2007) MNRAS, 375, p. 665
  • Panaitescu, A., Kumar, P., (2001) ApJ, 560, pp. L49
  • Patton, D.R., Grant, J.K., Simard, L., Pritchet, C.J., Carlberg, R.G., Borne, K.D., (2005) AJ, 130, p. 2043
  • Pélangeon, A., (2008) A&A, 491, p. 157
  • Perez, J., Tissera, P., Blaizot, J., (2009) MNRAS, 397, p. 748
  • Perez, M.J., Tissera, P.B., Scannapieco, C., Lambas, D.G., De Rossi, M.E., (2006) A&A, 459, p. 361
  • Poggianti, B., (2009) ApJ, 693, p. 112
  • Pontzen, A., (2009), (arXiv:0909.1321); Prochaska, J.X., (2004) ApJ, 611, p. 200
  • Salpeter, E.E., (1955) ApJ, 121, p. 161
  • Salvaterra, R., Chincarini, G., (2007) ApJ, 656, pp. L49
  • Sánchez, A.G., Baugh, C.M., Percival, W.J., Peacock, J.A., Padilla, N.D., Cole, S., Frenk, C.S., Norberg, P., (2006) MNRAS, 366, p. 189
  • Savaglio, S., (2006) New J. Phys., 8, p. 195
  • Savaglio, S., Glazebrook, K., Le Borgne, D., (2009) ApJ, 691, p. 182
  • Scannapieco, C., Tissera, P.B., White, S.D.M., Spirngel, V., (2005) MNRAS, 364, p. 552
  • Scannapieco, C., Tissera, P.B., White, S.D.M., Springel, V., (2006) MNRAS, 371, p. 1125
  • Springel, V., (2005) MNRAS, 364, p. 1105
  • Springel, V., Hernquist, L., (2003) MNRAS, 339, p. 289
  • Springel, V., White, S.D.M., Tormen, G., Kauffmann, G., (2001) MNRAS, 328, p. 726
  • Springel, V., (2005) Nat, 435, p. 629
  • Stern, B., Tikhomirova, Y., Kompaneets, D., Svensson, R., Poutanen, J., (2001) ApJ, 563, p. 80
  • Thöne, Ch.C., (2008) ApJ, 676, p. 1151
  • Wainwright, C., Berger, E., Penprase, B.E., (2007) ApJ, 657, p. 367
  • Wang, J., De Lucia, G., Kitzbichler, M.G., White, S.D.M., (2008) MNRAS, 384, p. 1301
  • Weinmann, S., Van Den Bosch, F.C., Yang, X., Mo, H.J., (2006) MNRAS, 366, p. 2
  • White, S.D.M., Frenk, C.S., (1991) ApJ, 379, p. 52
  • Wijers, R.A.M.J., Bloom, J.S., Bagla, J.S., Natarajan, P., (1998) MNRAS, 294, pp. L13
  • Wolf, C.h., Podsiadlowski, P., (2007) MNRAS, 375, p. 1049
  • Woosley, S.E., (1993) ApJ, 405, p. 273
  • Yonetoku, D., Yamazaki, R., Nakamura, T., Murakami, T., (2005) MNRAS, 362, p. 1114
  • Yoon, S.C., Langer, N., Norman, C., (2006) A&A, 460, p. 199

Citas:

---------- APA ----------
Chisari, N.E., Tissera, P.B. & Pellizza, L.J. (2010) . Host galaxies of long gamma-ray bursts in the Millennium Simulation. Monthly Notices of the Royal Astronomical Society, 408(1), 647-656.
http://dx.doi.org/10.1111/j.1365-2966.2010.17169.x
---------- CHICAGO ----------
Chisari, N.E., Tissera, P.B., Pellizza, L.J. "Host galaxies of long gamma-ray bursts in the Millennium Simulation" . Monthly Notices of the Royal Astronomical Society 408, no. 1 (2010) : 647-656.
http://dx.doi.org/10.1111/j.1365-2966.2010.17169.x
---------- MLA ----------
Chisari, N.E., Tissera, P.B., Pellizza, L.J. "Host galaxies of long gamma-ray bursts in the Millennium Simulation" . Monthly Notices of the Royal Astronomical Society, vol. 408, no. 1, 2010, pp. 647-656.
http://dx.doi.org/10.1111/j.1365-2966.2010.17169.x
---------- VANCOUVER ----------
Chisari, N.E., Tissera, P.B., Pellizza, L.J. Host galaxies of long gamma-ray bursts in the Millennium Simulation. Mon. Not. R. Astron. Soc. 2010;408(1):647-656.
http://dx.doi.org/10.1111/j.1365-2966.2010.17169.x