Chemical evolution of milky way type galaxies in the millennium simulation
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...
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| Otros Autores: | , , |
| Formato: | Acta de conferencia Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
Universidad Nacional Autonoma de Mexico
2009
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| Acceso en línea: | Registro en Scopus Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 03910caa a22004937a 4500 | ||
|---|---|---|---|
| 001 | PAPER-23273 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250219085131.0 | ||
| 008 | 190411s2009 xx ||||fo|||| 10| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-70749128417 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a De Rossi, María Emilia | |
| 245 | 1 | 0 | |a Chemical evolution of milky way type galaxies in the millennium simulation |
| 260 | |b Universidad Nacional Autonoma de Mexico |c 2009 | ||
| 270 | 1 | 0 | |m De Rossi, M. E.; Consejo Nacional de Investigaciones CientíFisica Técnicas, Ciudad de Buenos Aires, Argentina; email: derossi@iafe.uba.ar |
| 504 | |a Croton, D.J., (2006) MNRAS, 365, p. 11 | ||
| 504 | |a De Lucia, G., Blaizot, J., (2007) MNRAS, 375, p. 2 | ||
| 504 | |a De Rossi, M.E., Tissera, P.B., Scannapieco, C., (2007) MNRAS, 374, p. 323 | ||
| 504 | |a Erb, D.K., (2006) ApJ, 644, p. 813 | ||
| 504 | |a Lee, H., (2006) ApJ, 647, p. 970 | ||
| 504 | |a Lemson, G., (2006), & the Virgo Consortium, preprint astro-ph/0608019; Savaglio, S., (2005) ApJ, 635, p. 260 | ||
| 504 | |a Simien, F., de Vaucouleurs, G., (1986) ApJ, 302, p. 564 | ||
| 504 | |a Springel, V., (2005) Nature, 435, pp. 629S | ||
| 504 | |a Tissera, P.B., De Rossi, M.E., Scannapieco, C., (2005) MNRAS, 364, pp. L38 | ||
| 504 | |a 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) | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a 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. |l eng | |
| 593 | |a Consejo Nacional de Investigaciones CientíFisica Técnicas, Ciudad de Buenos Aires, Argentina | ||
| 593 | |a Instituto de Astronomía Física del Espacio, Casilla de Correos 67, Suc. 28, 1428, Ciudad de Buenos Aires, Argentina | ||
| 593 | |a Max-Planck-Institut fíur Astrophysik, Karl- Schwarzschild-Str. 1, Postfach 13 17, 85741, Garching bei Míunchen, Germany | ||
| 690 | 1 | 0 | |a COSMOLOGY: THEORY |
| 690 | 1 | 0 | |a GALAXIES: ABUNDANCES |
| 690 | 1 | 0 | |a GALAXIES: EVOLUTION |
| 690 | 1 | 0 | |a GALAXIES: FORMATION |
| 700 | 1 | |a De Lucia, Gabriela | |
| 700 | 1 | |a Tissera, P.B. | |
| 700 | 1 | |a Kaumann, G. | |
| 711 | 2 | |c Isla Margarita |d 22 October 2007 through 26 October 2007 | |
| 773 | 0 | |d Universidad Nacional Autonoma de Mexico, 2009 |g v. 35 |h pp. 213-214 |p Rev.Mex. Astron. Astrofis. Ser. Conf. |n Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |x 14052059 |w (AR-BaUEN)CENRE-1052 |t 12th IAU Regional Latin American Meeting of Astronomy | |
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| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_14052059_v35_n_p213_DeRossi |x handle |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v35_n_p213_DeRossi |x registro |y Registro en la Biblioteca Digital |
| 961 | |a paper_14052059_v35_n_p213_DeRossi |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/conferenceObject |a info:ar-repo/semantics/documento de conferencia |b info:eu-repo/semantics/publishedVersion | ||