Hostname: page-component-76fb5796d-25wd4 Total loading time: 0 Render date: 2024-04-26T16:02:55.271Z Has data issue: false hasContentIssue false
  • English
  • Français

Chemical Evolution of the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

B. Barbuy ,
J. A. de Freitas Pacheco  and
T. Idiart
B. Barbuy
Affiliation:
Universidade de São Paulo C.P. 3386, Sao Paulo 01060-970, Brazil
J. A. de Freitas Pacheco
Affiliation:
Observatoire de la Côte d'azur BP 4229, 06304 Nice Cedex 4, Prance
T. Idiart
Affiliation:
Observatoire de la Cote d'Azur BP 4229, 06304 Nice Cedex 4, Prance

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Chemical evolution studies of the Clouds based on detailed abundance analyses are essentially limited nowadays to young objects like HII regions (Dufour 1984; Garnett et al. 1995), planetary nebulae (e.g. de Freitas Pacheco et al. 1993), supernova remnants (Russell & Dopita 1990) and supergiant stars either of F-K type (Hill et al. 1995) or B ones (e.g. Rolleston et al. 1996 and references therein). One exception to this was presented by Dopita et al. (1997) where HST data permitted to date planetary nebulae nuclei and to present an age vs. metallicity model.

Type
Conference Papers in order of Presentation
Information
Symposium - International Astronomical Union , Volume 187: Cosmic Chemical Evolution , 2002 , pp. 195 - 199
Copyright
Copyright © 2002 

References

Ardeberg, A., Gustafsson, B., Nissen, P.-E. 1997 A&A, 322, L13.Google Scholar
Bertelli, G., Mateo, M., Chiosi, C., Bressan, A. 1992, ApJ, 388, 400.Google Scholar
Bica, E., Alloin, D., Santos, J.F.C. Jr. 1990: A&A, 235, 103.Google Scholar
Borges, A.C., Idiart, T.P., de Freitas Pacheco, J. A., & Thevenin, F. 1995, AJ, 110, 2408.Google Scholar
Dopita, et al. 1997, ApJS, 108, 515.CrossRefGoogle Scholar
Dufour, R.J. 1984, in Structure and evolution of the Magellanic Clouds , IAU Symp. 108, eds. van den Bergh, S., de Boers, K., Reidel (Dordrecht), p. 353.CrossRefGoogle Scholar
Elson, R., Fall, M. 1985, ApJ, 299, 211.Google Scholar
Elson, R., Gilmore, G., Santiago, B. 1997, MNRAS, in press.Google Scholar
Faber, S.M., Friel, E.D., Burstein, D., & Gaskell, C.M. 1985, ApJS 57, 711.Google Scholar
Frenk, C., Fall, M. 1982, MNRAS, 199, 565.Google Scholar
de Freitas Pacheco, J.A., Barbuy, B., Costa, R.D.D., & Idiart, T. 1993, A&A, 271, 429.Google Scholar
Frogel, J., Persson, S.E., Cohen, J.G. 1983, ApJS, 53, 71.CrossRefGoogle Scholar
de Freitas Pacheco, J.A. 1997, A&A, 319, 394.Google Scholar
Gallagher, et al. 1996, ApJ, 466, 732.Google Scholar
Garnett, D.R., Skillman, E.D., Dufour, R.J., Peimbert, M., Torres-Peimbert, S., Terlevich, R., Terlevich, E., & Shields, G.A. 1995, ApJ, 443, 64.Google Scholar
Girardi, L., Bica, E. 1993, A&A 274, 279.Google Scholar
Girardi, L., Chiosi, C., Bertelli, G., Bressan, A. 1995, A&A 298, 87.Google Scholar
Hill, V., Andrievsky, S., & Spite, M. 1995, A&A, 293, 347.Google Scholar
Hill, V., Barbuy, B., Spite, M. 1997, A&A, 323, 461.Google Scholar
Lequeux, J. 1993, ESO/OHP workshop on Dwarf Galaxies, eds. Meylan, G. & Prugniel, P., ESO/CNRS, p. 179.Google Scholar
Nomoto, K., Thielemann, F.-K., Yokoi, K. 1984, ApJ, 286, 644.Google Scholar
Olszewski, E.W., Schommer, R.A., Suntzeff, N., & Harris, H.C. 1991, AJ, 101, 515.Google Scholar
Persson, S.E., Aaronson, M., Cohen, J.G., Frogel, J.A., & Matthews, K. 1983, ApJ, 266, 105.CrossRefGoogle Scholar
Rolleston, W., Brown, P., Dufton, P., Howarth, I. 1996, A&A, 315, 95.Google Scholar
Russell, S.C., Dopita, M.A. 1990, ApJ, 384, 508.CrossRefGoogle Scholar
Stappers, et al. 1997, PASP, 109, 292.Google Scholar
Thielemann, F.-K., Nomoto, K., Hashimoto, M. 1996, ApJ, 460, 408.Google Scholar
Vallenari, A., Chiosi, C., Bertelli, G., Ortolani, S. 1996, A&A, 309, 358.Google Scholar
Westerlund, B., Linde, P., Lynga, G. 1995, A&A, 298, 39.Google Scholar