Abstract:
Using a Salpeter initial mass function (IMF) allows to describe fairly well a large variety of properties in galaxies. However, some studies have found that it is necessary to change it for a top-heavy IMF in starbursts to give an adequate prediction in the abundance of submillimeter galaxies (SMGs) at high redshifts. We show preliminary results of an implementation of a star formation intensity dependent IMF slope in a semi-analytic model of galaxy formation, which has been connected with a spectrophotometric code that provides an adequate treatment of reprocessed starlight by dust. We also explore systematic effects on the counts of submm sources coming from the beamsize of the receiver taking into account the spatial correlation of sources and foreground objects. This helps alleviate the discrepancies found between the model and the observations. © 2011: Instituto de Astronomía.
Registro:
Documento: |
Conferencia
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Título: | A variable IMF slope to fit the LCDM picture to observed high-Z submillimeter sources |
Autor: | Muñoz, A.M.; Navarrete, F.P.; Del P. Lagos, C.; Padilla, N.D.; Cora, S.A.; Tecce, T.E. |
Ciudad: | Morelia, Michoacan |
Filiación: | Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicunã Mackenna 4860, Santiago, Chile Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Institute for Computational Cosmology, Durham University, Durham DH1 3LE, United Kingdom Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Instituto de Astrofísica de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina IAFE, CONICET/UBA, CC 67 Suc. 28, C1428ZAA Buenos Aires, Argentina
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Palabras clave: | Galaxies: Evolution; Galaxies: High-redshift; Methods: Numerical; Submillimeter: Galaxies |
Año: | 2011
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Volumen: | 40
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Página de inicio: | 21
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Página de fin: | 22
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Título revista: | 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010
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Título revista abreviado: | Rev.Mex. Astron. Astrofis. Ser. Conf.
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ISSN: | 14052059
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p21_Munoz |
Referencias:
- Baugh, C.M., (2005) MNRAS, 356, p. 1191. , (B05)
- Bruzual, G., Charlot, S., (1993) ApJ, 405, p. 538
- Hughes, D.H., (1998) Nature, 394, p. 241
- Lagos, C., (2008) MNRAS, 388, p. 587. , (LCP08)
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- Weidner, C., Kroupa, P., (2006) MNRAS, 365, p. 1333. , (WK06)A4 - International Astronomical Union (IAU); CIC-UNAM and (CRyA-UNAM); Mexican National Science and Technology Council (CONACyT); Michoacan State Government; Michoacan State Science and Technology Council (COECyT)
Citas:
---------- APA ----------
Muñoz, A.M., Navarrete, F.P., Del P. Lagos, C., Padilla, N.D., Cora, S.A. & Tecce, T.E.
(2011)
. A variable IMF slope to fit the LCDM picture to observed high-Z submillimeter sources. 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010, 40, 21-22.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p21_Munoz [ ]
---------- CHICAGO ----------
Muñoz, A.M., Navarrete, F.P., Del P. Lagos, C., Padilla, N.D., Cora, S.A., Tecce, T.E.
"A variable IMF slope to fit the LCDM picture to observed high-Z submillimeter sources"
. 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010 40
(2011) : 21-22.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p21_Munoz [ ]
---------- MLA ----------
Muñoz, A.M., Navarrete, F.P., Del P. Lagos, C., Padilla, N.D., Cora, S.A., Tecce, T.E.
"A variable IMF slope to fit the LCDM picture to observed high-Z submillimeter sources"
. 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010, vol. 40, 2011, pp. 21-22.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p21_Munoz [ ]
---------- VANCOUVER ----------
Muñoz, A.M., Navarrete, F.P., Del P. Lagos, C., Padilla, N.D., Cora, S.A., Tecce, T.E. A variable IMF slope to fit the LCDM picture to observed high-Z submillimeter sources. Rev.Mex. Astron. Astrofis. Ser. Conf. 2011;40:21-22.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p21_Munoz [ ]