Abstract:
We have studied the origin of the Tully-Fisher relation by analysing hydrodynamical simulations in a ΔCDM universe. We found that smaller galaxies exhibit lower stellar masses than those predicted by the linear fit to high mass galaxies (fast rotators), consistently with observations. In this model, these trends are generated by the more efficient action of supernova feedback in the regulation of the star formation in smaller galaxies. Without introducing scale-dependent parameters, the model predicts that the Tully-Fisher relation bends at a characteristic velocity of ∼100 km s-1, in agreement with previous observational and theoretical findings. © 2011: Instituto de Astronomía.
Registro:
Documento: |
Conferencia
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Título: | Supernova feedback and the bend of the Tully-Fisher relation |
Autor: | De Rossi, M.E.; Tissera, P.B.; Pedrosa, S.E. |
Ciudad: | Morelia, Michoacan |
Filiación: | Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC 67, Suc 28 (1428), Buenos Aires, Argentina Consejo Nacional de Investigaciones Científicas y Técnicas, Buenos Aires, Argentina Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Buenos Aires, Argentina
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Palabras clave: | Cosmology: Theory; Galaxies: Evolution; Galaxies: Formation |
Año: | 2011
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Volumen: | 40
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Página de inicio: | 56
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Página de fin: | 57
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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_p56_DeRossi |
Referencias:
- Dekel, A., Silk, J., (1986) ApJ, 303, p. 39
- De Rossi, M.E., Tissera, P.B., Pedrosa, S.E., (2010) A & A, 519, p. 89
- Larson, R.B., (1974) MNRAS, 169, p. 229
- McGaugh, S.S., Schombert, J.M., Bothun, G.D., De Blok, W.J.G., (2000) ApJ, 533, pp. L99
- McGaugh, S.S., Schombert, J.M., De Blok, W.J.G., Zagursky, M.J., (2010) ApJ, 708, pp. L14
- Scannapieco, C., Tissera, P.B., White, S.D.M., Springel, V., (2006) MNRAS, 371, p. 1125A4 - 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 ----------
De Rossi, M.E., Tissera, P.B. & Pedrosa, S.E.
(2011)
. Supernova feedback and the bend of the Tully-Fisher relation. 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010, 40, 56-57.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p56_DeRossi [ ]
---------- CHICAGO ----------
De Rossi, M.E., Tissera, P.B., Pedrosa, S.E.
"Supernova feedback and the bend of the Tully-Fisher relation"
. 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010 40
(2011) : 56-57.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p56_DeRossi [ ]
---------- MLA ----------
De Rossi, M.E., Tissera, P.B., Pedrosa, S.E.
"Supernova feedback and the bend of the Tully-Fisher relation"
. 13th Latin American Regional Meeting of the International Astronomical Union, LARIM 2010, vol. 40, 2011, pp. 56-57.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p56_DeRossi [ ]
---------- VANCOUVER ----------
De Rossi, M.E., Tissera, P.B., Pedrosa, S.E. Supernova feedback and the bend of the Tully-Fisher relation. Rev.Mex. Astron. Astrofis. Ser. Conf. 2011;40:56-57.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p56_DeRossi [ ]