Abstract
We reconstruct the history of the cosmic star formation as well as the cosmic production of metals in the universe by means of detailed chemical evolution models for galaxies of different morphological types. We consider a picture of coeval, non-interacting evolving galaxies where ellipticals experience intense and rapid starbursts within the first Gyr after their formation, and spirals and irregulars continue to form stars at lower rates up to the present time. We show that spirals are the main contributors to the decline of the luminosity density in all bands between z=1 and z=0.
Similar content being viewed by others
References
Calura, F., Matteucci, F. and Vladilo, G.: 2002, MNRAS, in press, astro-ph/0211153.
Connolly, A.J. et al.: 1997, ApJ 486, L11.
Ellis, R.S. et al.: 1996, MNRAS 280, 235.
Gardner, J.P.: 1997, ApJ 480, L99.
Jimenez, R. et al.: 1998, MNRAS 299, 123.
Lilly, S. et al.: 1996, ApJ 460, L1.
Madau, P., Pozzetti, L. and Dickinson, M.: 1998, ApJ 498, 106.
Marzke, R.O. et al.: 1998, ApJ 503, 617.
Massarotti, M. et al.: 2002, ApJ 559, L105.
Pascarelle, S.M. et al.: 1998, ApJ 508, L1.
Pettini, M.: 1999, astro-ph/9902173.
Péroux, C. et al., astro-ph/0107045.
Rao, S. and Briggs, F.: 1993, ApJ 419, 515.
Rao, S. and Turnshek, D.A.: 2000, ApJS 130, 1.
Rosenberg, J. and Schneider, S.E.: 2002, ApJ 567, 247.
Somerville, R. et al.: 2001, MNRAS 320, 504.
Treyer, M.A. et al.: 1998, MNRAS 300, 303.
Zwaan, M.A. et al.: 1997, ApJ 490, 173.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Calura, F., Matteucci, F. The evolution of cosmic star formation, metals and gas. Astrophysics and Space Science 284, 429–432 (2003). https://doi.org/10.1023/A:1024023320657
Issue Date:
DOI: https://doi.org/10.1023/A:1024023320657