Hostname: page-component-76fb5796d-2lccl Total loading time: 0 Render date: 2024-04-27T00:52:09.628Z Has data issue: false hasContentIssue false

Comparing Chemical Abundances of the Damped Lyα Systems and Metal-Poor Stars

Published online by Cambridge University Press:  30 March 2016

Jason X. Prochaska*
Affiliation:
UCO/Lick Observatory, UC Santa Cruz, Santa Cruz, CA, 95064

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.

I briefly draw comparisons between the fields of damped Lyα and metal-poor stellar abundances. In particular, I examine their complementary age-metallicity relations and comparisons between the damped Lyα and dwarf galaxy abundance patterns. Regarding the latter, I describe a series of problems concerning associating high z damped Lyα systems with present-day dwarfs.

Type
I. Joint Discussions
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Dessauges-Zavadsky, M. et al. 2003, MNRAS, 345, 447 CrossRefGoogle Scholar
Edvardsson, B., Andersen, J., Gustafsson, B. et al. 1993, A&A, 275, 101 Google Scholar
Feltzing, S., Holmberg, J., & Hurley, J.R. 2001, A&A, 377, 911 Google Scholar
Haehnelt, M.G., Steinmetz, M. & Rauch, M. 1998, ApJ, 495, 647 CrossRefGoogle Scholar
Ibukiyama, A. & Arimoto, N. 2002, A&A, 394, 927 Google Scholar
Jenkins, E.B. 1987, in Interstellar Processes, ed. Hollenbach, D.J. and Thronson, H.A. Jr. (Boston: D. Reidel Publishing Company), p. 533 Google Scholar
Kulkarni, V. P. 2003, This proceedings, JD 15Google Scholar
Maller, A.H., Prochaska, J.X., Somerville, R.S., & Primack, J.R. 2001, MNRAS, 326, 1475 CrossRefGoogle Scholar
McWilliam, A., Preston, G.W., Sneden, C., & Searle, L. 1995, AJ, 109, 2757 CrossRefGoogle Scholar
Pettini, M., Smith, L.J., King, D.L., & Hunstead, R.W. 1997, ApJ, 486, 665 CrossRefGoogle Scholar
Prochaska, J.X., Howk, J.C., O’Meara, J.M. et al. 2002, ApJ, 571, 693 CrossRefGoogle Scholar
Prochaska, J.X., Gawiser, E., Wolfe, et al. 2003, ApJ, 595, L9 CrossRefGoogle Scholar
Prochaska, J.X., Howk, J.C., & Wolfe, A.M. 2003, Nature, 423, 57 CrossRefGoogle Scholar
Prochaska, J.X. & Wolfe, A. M. 1997, ApJ, 486, 73 CrossRefGoogle Scholar
Prochaska, J.X. & Wolfe, A.M. 2002, ApJ, 566, 68 CrossRefGoogle Scholar
Rocha-Pinto, H.J., Scalo, J., Maciel, W.J., & Flynn, C. 2000, A&A, 358, 869 Google Scholar
Savage, B. D.and Sembach, K. R. 1996, ARA&A, 34, 279 Google Scholar
Shetrone, M., Côté, P., Sargent, W.L.W. 2001, ApJ, 548, 592 CrossRefGoogle Scholar
Spergel, D.N., et al. 2003, ApJS, 148, 175 CrossRefGoogle Scholar
Tolstoy, E., Venn, K.A., Shetrone, M. et al. 2003, AJ, 125, 707 CrossRefGoogle Scholar
Venn, K.A., Tolstoy, E., Kaufer, A. et al. 2003, AJ, 126, 1326 CrossRefGoogle Scholar
Vladilo, G., Centurion, M., Bonifacio, P., & Howk, J.C. 2001, ApJ, 557, 1007 CrossRefGoogle Scholar
Vladilo, G. 2002, A&A, 391, 407 Google Scholar
Wolfe, A. M. 2003, This proceedings, JD 15Google Scholar