Chemical evolution of the galactic disk via simulations of the open cluster system
We present numerical simulations of the system of open clusters of the Milky Way, whose aim is to provide constraints on the evolution of the star formation rate and the metallicity of the galactic disk. We find that the properties of the open cluster system are well described assuming an almost con...
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| Otros Autores: | , |
| Formato: | Acta de conferencia Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2006
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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 | 03896caa a22005057a 4500 | ||
|---|---|---|---|
| 001 | PAPER-21706 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205311.0 | ||
| 008 | 190411s2006 xx ||||fo|||| 10| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-34548539851 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Tecce, T.E. | |
| 245 | 1 | 0 | |a Chemical evolution of the galactic disk via simulations of the open cluster system |
| 260 | |c 2006 | ||
| 270 | 1 | 0 | |m Tecce, T. E.; Instituto de Astronomía y Física del Espacio( CONICET-UBA), C.C. 67 Suc. 28 (1428) Ciudad Universitaria, Buenos Aires, Argentina; email: tomas@iafe.uba.ar |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Chen, L., Hou, J.L., Wang, J.J., (2003) AJ, 125, p. 1397 | ||
| 504 | |a Chiappini, C., Matteucci, F., Romano, D., (2001) ApJ, 554, p. 1044 | ||
| 504 | |a Dehnen, W., Binney, J., (1998) MNRAS, 294, p. 429 | ||
| 504 | |a Feltzing, S., Holmberg, J., Hurley, J.R., (2001) A&A, 377, p. 911 | ||
| 504 | |a Kennicutt, R.C., (1998) ApJ, 498, p. 541 | ||
| 504 | |a Kharchenko, N.V., Piskunov, A.E., Röser, S., Schilbach, E., Scholz, R.-D., (2005) A&A, 438, p. 1163 | ||
| 504 | |a Lamers, H.J.G.L., Gieles, M., Bastian, N., Baumgardt, H., Kharchenko, N.V., Portegies Zwart, S., (2005) A&A, 441, p. 117 | ||
| 504 | |a Piatti, A.E., Clariá, J.J., Abadi, M.G., (1995) AJ, 110, p. 2813 | ||
| 504 | |a Rocha-Pinto, H.J., Maciel, W.J., Scalo, J.M., Flynn, C., (2000) A&A, 358, p. 850 | ||
| 504 | |a Scalo, J.M., in Starbursts and Galaxy (1987) Evolution, p. 445 | ||
| 504 | |a Soderblom, D.R., Duncan, D.K., Johnson, D.R.H., (1991) ApJ, 375, p. 722 | ||
| 504 | |a Tecce, T. E., Pellizza, L. J., & Piatti, A. E. 2006, BAAA, submitted; Twarog, B.A., (1980) ApJ, 242, p. 242A4 - Universidad de Chile (U); Pontificia Universidad Catolica (PUC); Universidad de Concepcion (UCon); Ministerio de Relaciones Exteriores de Chile (MINREL); Consejo Nacional de Ciencia y Tecnologia (CONACyT) | ||
| 520 | 3 | |a We present numerical simulations of the system of open clusters of the Milky Way, whose aim is to provide constraints on the evolution of the star formation rate and the metallicity of the galactic disk. We find that the properties of the open cluster system are well described assuming an almost constant SFR for the disk, a primordial radial metallicity gradient which remains the same at all times, and the inexistence of an age-metallicity relationship. © 2006: Instituto de Astronomía. |l eng | |
| 593 | |a Instituto de Astronomía y Física del Espacio( CONICET-UBA), C.C. 67 Suc. 28 (1428) Ciudad Universitaria, Buenos Aires, Argentina | ||
| 593 | |a AIM - Astrophysique Interactions Multi-́echelles, CEA Saclay, DSM/DAPNIA/Service d'Astrophysique, Bât. 709, L'Orme des Merisiers, Gif-sur-Yvette, 91191, France | ||
| 690 | 1 | 0 | |a GALAXY: DISK |
| 690 | 1 | 0 | |a GALAXY: EVOLUTION |
| 690 | 1 | 0 | |a METHODS: NUMERICAL |
| 690 | 1 | 0 | |a OPEN CLUSTERS AND ASSOCIATIONS: GENERAL |
| 700 | 1 | |a Pellizza, L.J. | |
| 700 | 1 | |a Piatti, A.E. | |
| 711 | 2 | |c Pucon |d 12 December 2005 through 16 December 2005 | |
| 773 | 0 | |d 2006 |g v. 26 |h pp. 86-87 |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 XI IAU Regional Latin American Meeting of Astronomy, LARIM2005 | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-34548539851&partnerID=40&md5=487deb5ed7cae5fee6a9b4129eb7407c |y Registro en Scopus |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_14052059_v26_n_p86_Tecce |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v26_n_p86_Tecce |y Registro en la Biblioteca Digital |
| 961 | |a paper_14052059_v26_n_p86_Tecce |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 | ||
| 999 | |c 82659 | ||