Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-14T09:11:24.889Z Has data issue: false hasContentIssue false
  • English
  • Français

UV to IR Models of Galaxy Evolution and Cosmology

Published online by Cambridge University Press:  07 August 2017

Brigitte Rocca-Volmerange
Brigitte Rocca-Volmerange*
Affiliation:
Institut d'Astrophysique 98 bis Bd Arago F-75014 PARIS

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.

Recent improvements of spectrophotometric evolutionary models are described. New stellar libraries in the near-infrared (JHK) allow extension of the synthetic spectral Atlas of galaxies down to 10μm. From analyses in the far-UV and visible, observed colors and counts of faint galaxies are fitted by modelling a standard luminosity evolution and a low value of ωo(≃ 0.1) while, in a ωo=1 Universe, models only fit data with a standard luminosity evolution and a number density evolution ≃ (1 + z)1.8: such a modelling is simulating a merging process. Another solution would be a tidally triggered star formation rate in a model in which galaxies form by hierarchical clustering of a dominant dark matter component. From evolution of M/L ratio, these models allow to link observed luminosity functions with mass distributions predicted from galaxy formation models and then to significantly connect evolution to formation models. Nevertheless these two models are not sufficient to fit some observational data such as the Hubble diagrams and faint galaxy counts in the near-infrared, the bright galaxy counts in visible and the Extragalactic Background Light. So new evolution scenarios are needed implying other constraints for cosmological parameters.

Type
III. The Stellar Populations of Non-Resolved Galaxies
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 357 - 366
Copyright
Copyright © Kluwer 

References

Arimoto, N., Yoshii, Y., 1986, Astron. Astrophys. , 164, 260.Google Scholar
Bardeen, J.M., Bond, J.R., Kaiser, N., Szalay, A.S., 1986, Astrophys. J. , 304, 15.Google Scholar
Baron, E. & White, S.D.M., 1987. Astrophys. J. 322, 585.Google Scholar
Bithell, M. & Rees, M.J., 1990. Mon. Not. R. astr. Soc. 242, 570.CrossRefGoogle Scholar
Broadhurst, T.J., Ellis, R.S. & Shanks, T., 1988. Mon. Not. R. astr. Soc. 235, 827.Google Scholar
Bruzual, G., 1983. Astrophys. J. 273, 105.Google Scholar
Butcher, H.R., Oemler, A., 1978, Astrophys. J. , 219, 18.Google Scholar
Carlberg, R.G., 1985, in the Milky way Galaxy , van Woerden, H., Allen, R.J., Burton, W.B. (ed), Dordrecht, Reidel, p.165.Google Scholar
Carlberg, R.G. & Couchman, H.M.P., 1989. Astrophys. J. 340, 47.Google Scholar
Chambers, K.C., Miley, G.K. & van Breugel, R.R., 1988. Astrophys. J. 329, L75.Google Scholar
Chambers, K.C. & Charlot, S, 1990. Astrophys. J. 348, L1.Google Scholar
Clegg, R.E.S., Middlemass, D., 1987, Mon. N. Roy. astr. Soc. , 244, 408.Google Scholar
Colless, M., Ellis, R.S., Taylor, K., Hook, R.N., 1990, Mon. N. Roy. astr. Soc. , 244, 408.Google Scholar
Cowie, L., Lilly, S., Gardner, J., 1991, preprint.Google Scholar
de Jager, C., Nieuwenhuijzen, H., van der Hucht, K.A., 1988, Astron. Astrophys. , 164, 260.Google Scholar
Djorgovski, S., Spinrad, H., Marr, J., 1984, in New Aspects of Galaxy Photometry, Nieto, J.L. (ed.), Springer–Verlag, p. 193.Google Scholar
Djorgovski, S., Spinrad, H., McCarthy, P., Dickinson, M., Van Breugel, W. & Strom, R.G., 1988. Astron. J. 96, 836.Google Scholar
Dressler, A., 1980, Astrophys. J. , 236, 351.Google Scholar
Dressler, A., Gunn, J.E., 1983, Astrophys.J. , 270, 7.Google Scholar
Evrard, A.E., 1989. Astrophys. J. 341, 26.Google Scholar
Franceschini, A., Toffolati, L., Mazzei, P., Danese, L., de Zotti, G., 1991, preprint.Google Scholar
Fukujita, F., Takahara, F., Yamashita, K., Yoshii, Y., 1990, Astrophys. J. , 361, L1.Google Scholar
Guiderdoni, B. & Rocca–Volmerange, B., 1984. Astron. Astrophys. 109, 355.Google Scholar
Guiderdoni, B. & Rocca–Volmerange, B., 1987. Astron. Astrophys. 186, 1.Google Scholar
Guiderdoni, B. & Rocca–Volmerange, B., 1990. Astron. Astrophys. 227, 362.Google Scholar
Guiderdoni, B., Rocca–Volmerange, B., 1991, in press.Google Scholar
Heck, A., Egret, D., Jaschek, C., 1984, Battrick., B., ESA SP-1052.Google Scholar
Hintzen, P., Romanishin, W. & Valdes, F., 1991, Astrophys. J. 366, 7.Google Scholar
Huchra, J.P., 1977, Astrophys. J., 217, 928.Google Scholar
IUE Ultraviolet Spectral Atlas, 1983, Wu, et al., NASA N022.Google Scholar
Joy, M., Harvey, P.M., Tollestrup, E.P., Sellgren, K., Mc Gregor, P.J., Hyland, A.R., 1991, Astrophys. J. , 366, 82.Google Scholar
Kudritski, R.P., in Massive stars in starbursts , Leitherer, C. (ed), Baltimore, in press.Google Scholar
Lacey, C., Silk, J., 1991, in press.Google Scholar
Lacey, C., Guiderdoni, B., Rocca-Volmerange, B., Silk, J., submitted.Google Scholar
Lançon, A., Rocca-Volmerange, B., Maillard, J.P., 1991, submitted.Google Scholar
Larson, R., 1975, Mon. Not. R. astr. Soc. 173, 671.Google Scholar
Le Fèvre, O., Hammer, F. & Jones, J., 1988. Astrophys. J. 331, L73.Google Scholar
Lilly, S., 1988. Astrophys. J. 333, 161.Google Scholar
Maddox, S.J., Efstathiou, G. & Sutherland, W.J., 1990, Mon. Not. R. astr. Soc. 211, 833.Google Scholar
Lilly, S., 1989. Astrophys. J. 340, 77.Google Scholar
Le Fèvre, O., Hammer, F. & Jones, J., 1988. Astrophys. J. 331, L73.Google Scholar
Lilly, S., 1988. Astrophys. J. 333, 161.Google Scholar
Maddox, S.J., Efstathiou, G. & Sutherland, W.J., 1990, Mon. Not. R. astr. Soc. 211, 833.Google Scholar
Maeder, A. & Meynet, G., 1988. Astron. Astrophys. Suppl. Ser. 76, 411.Google Scholar
Mattila, K., 1991, in The early universe from diffuse backgrounds , Rocca-Volmerange, , Deharveng, , Thanh Van, Tran (ed), Editions Frontières.Google Scholar
Mirabel, I. F., & Sanders, D.B., 1988, Astrophys. J. , 340, L53.Google Scholar
Olofsson, K., 1989, Astron. Astrophys. Supp. Ser. , 76, 317.Google Scholar
Rocca–Volmerange, B., 1988. The Messenger 53, 26.Google Scholar
Rocca–Volmerange, B. & Guiderdoni, B., 1988. Astron. Astrophys. Suppl. Ser. 75, 93.Google Scholar
Rocca–Volmerange, B., Guiderdoni, B., 1990, Month. Not. Roy. Astron. Soc. , 247, 166.Google Scholar
Rocca–Volmerange, B. & Gros, L., 1991, in preparation.Google Scholar
Sanders, D.B., Soifer, B.T., Elias, J.H., Madore, B.F., Matthews, K., Neugebauer, G., Scoville, N.Z., 1988, Astrophys. J. , 325, 74.Google Scholar
Searle, L., Sargent, W.L.W., Bagnuolo, W., 1973, Astrophys. J., 179, 427.Google Scholar
Silk, J., 1978, Astrophys. J. , 220, 378.Google Scholar
Tinsley, B.M., 1972, Astron. Astrophys. , 20, 383.Google Scholar
Toomre, A., Toomre, J., 1972, Astrophys. J. , 178, 623.Google Scholar
Tyson, A., 1988. Astron. J. 96, 1.Google Scholar
VandenBergh, D., Bell, R.A., Astrophys. Supp. Series , 58, 561.Google Scholar
Yoshii, Y., Takahara, F., 1988, Astrophys. J., 326, 1.Google Scholar
Zepf, S.E., Koo, D.C., 1989, Astrophys. J., 337, 34.Google Scholar