Abstract
I review recent results concerning the metal enrichment of the intergalactic medium and give arguments which allow to conclude that the heavy elements detected in the Lyα forest absorbers must have been produced and injected by a population of protogalaxies with typical mass ≈ 108 M⊙ at redshift z ≈ 10. In addition, I will discuss the existence of a metallicity-induced shift in the Initial Mass Function of first stars from an extrely top-heavy distribution to a `normal' one and bring observational support to this idea.
Similar content being viewed by others
References
Ciardi, B., Ferrara, A. and Abel, T.: 2000, ApJ 533, 594.
Ciardi, B., Ferrara, A., Governato, F. and Jenkins, A.: 2000, MNRAS 314, 611.
Bromm, V., Ferrara, A., Coppi, P.S. and Larson, R.B.: 2001, MNRAS 328, 969.
Ferrara, A., Pettini, M. and Shchekinov, Yu.: 2000, MNRAS 319, 539 (FPS).
Haiman, Z., Rees, M.J. and Loeb, A.: 1997, ApJ 476, 458.
Hernandez, X. and Ferrara, A.: 2001, MNRAS 324, 484.
Madau, P., Ferrara, A. and Rees, M.: 2001, ApJ, in press (astro-ph/0010158).
Mather, J.C., Fixsen, D.J., Shafer, R.A., Mosier, C. and Wilkinson, D.T.: 1999, ApJ 512, 511.
McKee, C.F. and Williams, J.P.: 1997, ApJ 476, 144.
Mori, M., Ferrara, A. and Madau, P.: 2001, ApJ, submitted (astro-ph/0106107).
Oey, Y.M.S. and Clarke, C.J.: 1997, MNRAS 289, 570.
Pettini, M.: 1999, in: J. Walsh and M. Rosa (eds.), Chemical Evolution from Zero to High Redshift, Springer, Berlin, p. 173.
Pagel, B.E.J.: 1998, in: D. Friedli, M. Edmunds, C. Robert and L. Drissen (eds.), Abundance Profiles: Diagnostic Tools for Galaxy History, ASP Conf. Ser. Vol. 147, San Francisco, ASP, p. 333.
Scannapieco, E., Ferrara, A. and Madau, P.: 2002, ApJ 574, 590.
Schneider, R., Ferrara, A., Natarayan, P. and Omukai, K.: 2002, ApJ 571, 30.
Steidel C.C. et al.: 1999, ApJ 519, 1.
White, S.D.M. and Rees, M.J.: 1978, MNRAS 183, 341.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ferrara, A. Pregalactic metal enrichment. Astrophysics and Space Science 284, 415–424 (2003). https://doi.org/10.1023/A:1024019202910
Issue Date:
DOI: https://doi.org/10.1023/A:1024019202910