Conferencia

De Rossi, M.E.; De Lucia, G.; Tissera, P.B.; Kaumann, G. "Chemical evolution of milky way type galaxies in the millennium simulation" (2009) 12th IAU Regional Latin American Meeting of Astronomy. 35:213-214
Estamos trabajando para incorporar este artículo al repositorio
Consulte la política de Acceso Abierto del editor

Abstract:

In this work we make use of the Millennium Run, which is at the moment the largest high-resolution simulation of structure formation ever carried out, combined with the semi-analytical model of De Lucia & Blaizot (2007), to follow the chemical evolution of Milky Way type galaxies with the aim at understanding their level of enrich- ment and the dispersion in the mass-metallicity correlation. Our results suggest that Milky Way type systems tend to evolve passively with time without su ing signi cant mass accretion. The chemical enrichment of these systems seems to be driven mainly by gas cooling, star formation efficiency and for the most massive progenitors by AGN feedback. © 2009: Instituto de Astronomía, UNAM.

Registro:

Documento: Conferencia
Título:Chemical evolution of milky way type galaxies in the millennium simulation
Autor:De Rossi, M.E.; De Lucia, G.; Tissera, P.B.; Kaumann, G.
Ciudad:Isla Margarita
Filiación:Consejo Nacional de Investigaciones CientíFisica Técnicas, Ciudad de Buenos Aires, Argentina
Instituto de Astronomía Física del Espacio, Casilla de Correos 67, Suc. 28, 1428, Ciudad de Buenos Aires, Argentina
Max-Planck-Institut fíur Astrophysik, Karl- Schwarzschild-Str. 1, Postfach 13 17, 85741, Garching bei Míunchen, Germany
Palabras clave:Cosmology: Theory; Galaxies: Abundances; Galaxies: Evolution; Galaxies: Formation
Año:2009
Volumen:35
Página de inicio:213
Página de fin:214
Título revista:12th IAU Regional Latin American Meeting of Astronomy
Título revista abreviado:Rev.Mex. Astron. Astrofis. Ser. Conf.
ISSN:14052059
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v35_n_p213_DeRossi

Referencias:

  • Croton, D.J., (2006) MNRAS, 365, p. 11
  • De Lucia, G., Blaizot, J., (2007) MNRAS, 375, p. 2
  • De Rossi, M.E., Tissera, P.B., Scannapieco, C., (2007) MNRAS, 374, p. 323
  • Erb, D.K., (2006) ApJ, 644, p. 813
  • Lee, H., (2006) ApJ, 647, p. 970
  • Lemson, G., (2006), & the Virgo Consortium, preprint astro-ph/0608019; Savaglio, S., (2005) ApJ, 635, p. 260
  • Simien, F., de Vaucouleurs, G., (1986) ApJ, 302, p. 564
  • Springel, V., (2005) Nature, 435, pp. 629S
  • Tissera, P.B., De Rossi, M.E., Scannapieco, C., (2005) MNRAS, 364, pp. L38
  • Tremonti, C.A., (2004) ApJ, 613, p. 898A4 - Centro de Investigaciones de Astronomia (CIDA); CorpoTur Nueva Esparta; et al.; Fondo Nacional de Ciencia y Tecnologia (FONACIT); Inst. Venez. Invest. Cient. (IVIC); Ministerio de Ciencia y Tecnologia (MCyT)

Citas:

---------- APA ----------
De Rossi, M.E., De Lucia, G., Tissera, P.B. & Kaumann, G. (2009) . Chemical evolution of milky way type galaxies in the millennium simulation. 12th IAU Regional Latin American Meeting of Astronomy, 35, 213-214.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v35_n_p213_DeRossi [ ]
---------- CHICAGO ----------
De Rossi, M.E., De Lucia, G., Tissera, P.B., Kaumann, G. "Chemical evolution of milky way type galaxies in the millennium simulation" . 12th IAU Regional Latin American Meeting of Astronomy 35 (2009) : 213-214.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v35_n_p213_DeRossi [ ]
---------- MLA ----------
De Rossi, M.E., De Lucia, G., Tissera, P.B., Kaumann, G. "Chemical evolution of milky way type galaxies in the millennium simulation" . 12th IAU Regional Latin American Meeting of Astronomy, vol. 35, 2009, pp. 213-214.
Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v35_n_p213_DeRossi [ ]
---------- VANCOUVER ----------
De Rossi, M.E., De Lucia, G., Tissera, P.B., Kaumann, G. Chemical evolution of milky way type galaxies in the millennium simulation. Rev.Mex. Astron. Astrofis. Ser. Conf. 2009;35:213-214.
Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v35_n_p213_DeRossi [ ]