Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-24T17:29:39.706Z Has data issue: false hasContentIssue false
  • English
  • Français

Global Evolution of the Stars, Gas, Metals, and Dust in Galaxies

Published online by Cambridge University Press:  19 July 2016

S. Michael Fall
S. Michael Fall*
Affiliation:
Space Telescope Science Institute 3700 San Martin Drive, Baltimore, MD 21218, USA

Abstract

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.

We outline a method to infer the global history of star formation in galaxies from absorption-line observations of quasars. The application to existing data leads to the conclusion that most stars formed at relatively low redshifts (z ≲ 2). The results obtained by this absorption-based method are consistent with those obtained subsequently by emission-based methods.

Type
Conference Papers in order of Presentation
Information
Symposium - International Astronomical Union , Volume 187: Cosmic Chemical Evolution , 2002 , pp. 201 - 207
Copyright
Copyright © 2002 

References

Connolly, A.J., Szalay, A.S., Dickinson, M., SubbaRao, M.U., & Brunner, R.J. 1997, ApJ, 486, L11.CrossRefGoogle Scholar
Fall, S.M., Chariot, S., & Pei, Y.C. 1996, ApJ, 464, L43.Google Scholar
Fall, S.M., & Pei, Y.C. 1993, ApJ, 402, 479.Google Scholar
Gallego, J., Zamorano, J., Aragón-Salamanca, A., & Rego, M. 1995, ApJ, 455, L1.Google Scholar
Ge, J., & Bechtold, J. 1997, ApJ, 477, L73.Google Scholar
Hartwick, F.D.A. 1976, ApJ, 209, 418.Google Scholar
Hauser, M.G. 1996, in Unveiling the Cosmic Infrared Background, ed. Dwek, E. (Woodbury: Am. Inst. Phys.), 11.Google Scholar
Kennicutt, R.C. 1989, ApJ, 344, 685.Google Scholar
Kulkarni, V.P., Fall, S.M., & Truran, J.W. 1997, ApJ, 484, L7.Google Scholar
Lanzetta, K.M., Wolfe, A.M., & Turnshek, D.A. 1995, ApJ, 440, 435.CrossRefGoogle Scholar
Larson, R.B. 1972, Nature Phys. Sci., 236, 7.CrossRefGoogle Scholar
Le Brun, V., Bergeron, J., Boissé, P., & Deharveng, J.M. 1997, A&A, 321, 733.Google Scholar
Levshakov, S.A., Chaffee, F.H., Foltz, C.B., & Black, J.H. 1992, A&A, 262, 385.Google Scholar
Lilly, S.J., Le Fèvre, O., Hammer, F., & Crampton, D. 1996, ApJ, 460, L1.Google Scholar
Lu, L., Sargent, W.L.W., Barlow, T.A., Churchill, C.W., & Vogt, S.S. 1996, ApJS, 107, 475.CrossRefGoogle Scholar
Madau, P., Ferguson, H.C., Dickinson, M.E., Giavalisco, M., Steidel, C.C., & Fruchter, A. 1996, MNRAS, 283, 1388.Google Scholar
Madau, P., Pozzetti, L., & Dickinson, M. 1998, ApJ, in press (astro-ph/9708220).Google Scholar
Pagel, B.E.J. 1997, Nucleosynthesis and Chemical Evolution of Galaxies (Cambridge: Cambridge University Press).Google Scholar
Pei, Y.C., & Fall, S.M. 1995, ApJ, 454, 69.Google Scholar
Pei, Y.C., Fall, S.M., & Bechtold, J. 1991, ApJ, 378, 6.Google Scholar
Perna, R., Loeb, A., & Bartelmann, M. 1997, ApJ, 488, 550.Google Scholar
Pettini, M., King, D.L., Smith, L.J., & Hunstead, R.W. 1997a, ApJ, 478, 536.Google Scholar
Pettini, M., Smith, L.J., Hunstead, R.W., & King, D.L. 1994, ApJ, 426, 79.Google Scholar
Pettini, M., Smith, L.J., King, D.L., & Hunstead, R.W. 1997b, ApJ, 486, 665.Google Scholar
Puget, J.-L., Abergel, A., Bernard, J.-P., Boulanger, F., Burton, W.B., Désert, F.-X., & Hartmann, D. 1996, A&A, 308, L5.Google Scholar
Shaver, P.A., Wall, J.V., Kellerman, K.I., Jackson, C.A., & Hawkins, M.R.S. 1996, Nature, 384, 439.Google Scholar
Smette, A., Claeskens, J.-F., & Surdej, J. 1997, New Astronomy, 2, 53.Google Scholar
Storrie-Lombardi, L.J., McMahon, R.G., & Irwin, M.J. 1996, MNRAS, 283, L79.Google Scholar
Vladilo, G. 1998, ApJ, 493, 583.Google Scholar
Welty, D.E., Lauroesch, J.T., Blades, J.C., Hobbs, L.M., & York, D.G. 1997, ApJ, 489, 672.Google Scholar
Wolfe, A.M., Lanzetta, K.M., Foltz, C.B., & Chaffee, F.H. 1995, ApJ, 454, 698.Google Scholar