Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-04T19:29:49.437Z Has data issue: false hasContentIssue false
  • English
  • Français

Chemical Constraints, Baryonic Mass and the Chemical Evolution of Low Surface Brightness Galaxies

Published online by Cambridge University Press:  12 April 2016

M.G. Edmunds
M.G. Edmunds*
Affiliation:
Department of Physics and Astronomy, Cardiff University, P.O. Box 913, Cardiff, CF2 3YB, U.K.

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.

A brief review of primordial helium and deuterium abundances suggests a baryonic mass density of ΩB ≈ 0.04 – 0.045 (for Ho = 70). This mass may be dominated by intergalactic gas in clusters and groups of galaxies. The observed low chemical abundances in evolved dwarf galaxies might suggest that outflow was the origin for such gas, and we make general suggestions for the interpretation of the data from the next generation of X-ray spectroscopic satellites. The effects of both outflow and inflow on the chemical evolution of galaxies is discussed, particularly in the context of low surface brightness galaxies, and we comment on their dust content.

Type
The baryonic mass content of the Universe
Information
International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 383 - 389
Copyright
Copyright © Astronomical Society of the Pacific 1999

References

Bristow, P.D. & Phillipps, S. 1994, MNRAS, 267, 13 CrossRefGoogle Scholar
Burles, S. & Tytler, D. 1998, ApJ, 507, 732 Google Scholar
de Blok, W.J.G. & van der Hulst, J.M. 1998, A&A, 335, 421 Google Scholar
Dwek, E. 1998, ApJ, 501, 643 Google Scholar
Edmunds, M.G. 1994, MNRAS, 270, L37 Google Scholar
Edmunds, M.G. 1999, MNRAS in preparation Google Scholar
Edmunds, & Eales, S.A. 1998, MNRAS, 299, L29 Google Scholar
Edmunds, M.G. & Phillipps, S. 1997, MNRAS, 292, 733 Google Scholar
Edmunds, M.G. & Roy, J-R., 1993, MNRAS, 261. L17 CrossRefGoogle Scholar
Fukugita, M., Hogan, C.J. & Peebles, P.J.E. 1998, ApJ, 503, 518 Google Scholar
Garnett, D.R., Shields, G.A., Skillman, E.D., Sagan, S.P. & Dufour, R.J. 1997. ApJ 489, 63 Google Scholar
Izotov, Y.I., Thuan, T.X. & Lipovetski, V.A. 1997, ApJS, 108, 1 Google Scholar
Köppen, J. & Edmunds, M.G. 1999, MNRAS, in press Google Scholar
McGaugh, S.S. 1994, ApJ, 426, 135 Google Scholar
McGaugh, S.S. & de Blok, W.J.G. 1997, 481, 689 Google Scholar
Pagel, B.E.J. 1997 Nucleosynthesis and the Chemical Evolution of Galaxies, Cambridge Univesity Press.Google Scholar
Pagel, B.E.J., Edmunds, M.G., Simonson, E.A. & Terlevich, R.J. 1992, MNRAS, 255, 325 CrossRefGoogle Scholar
Phillipps, S. & Edmunds, M.G. 1996, MNRAS, 281, 362 CrossRefGoogle Scholar
Ryder, S.D. 1995, ApJ, 444, 610 CrossRefGoogle Scholar
Tielens, A.G.G.M. 1998, ApJ, 499, 267 Google Scholar
Tosi, M., Steigman, G., Matteucci, F. & Chiappini, C. 1998, ApJ, 498, 226 CrossRefGoogle Scholar
Tytler, D., Fan, X.M. & Burles, S. 1996, Nature, 381, 207 Google Scholar
van Zee, L., Haynes, M.P. & Salzer, J.J. 1997, AJ, 114, 2497 Google Scholar
van Zee, L., Westpfahl, D., Haynes, M.P. & Salzer, J.J. 1998, AJ, 115, 1000 Google Scholar
Vila-Costas, M.B. & Edmunds, M.G. 1982, MNRAS 259, 121 Google Scholar
Vilchez, J.M. & Ingesias-Páramo, J. 1998, in Abundance Profiles: Diagnostic Tools for Galaxy History, ASP Conference Series, Vol 147 eds Friedli, D., Edmunds, M.G., C., Robert & Drissen, L. p120 Google Scholar
Wyse, R. & Silk, J. 1989, ApJ, 339, 700 Google Scholar