Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-28T00:12:38.372Z Has data issue: false hasContentIssue false
  • English
  • Français

Constraints on Elliptical Galaxy Formation from Dry Mergers

Published online by Cambridge University Press:  01 August 2006

Julia M. Comerford ,
Eliot Quataert  and
Chung-Pei Ma
Julia M. Comerford
Affiliation:
Astronomy Department, 601 Campbell Hall, University of California, Berkeley, CA 94720 email: [email protected]
Eliot Quataert
Affiliation:
Astronomy Department, 601 Campbell Hall, University of California, Berkeley, CA 94720 email: [email protected]
Chung-Pei Ma
Affiliation:
Astronomy Department, 601 Campbell Hall, University of California, Berkeley, CA 94720 email: [email protected]
Rights & Permissions [Opens in a new window]

Extract

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 observations suggest that dissipationless mergers of elliptical galaxies build up the population of massive early-type galaxies (Bell et al. 2004; Faber et al. 2006). This type of merger is observed in galaxy clusters (Tran et al. 2005) and predicted by semi-analytic models which find mass assembly times significantly later than star-formation times for the most massive elliptical galaxies (de Lucia & Blaizot 2006). Here, we use a semi-analytic model of minor mergers of dark matter halos to examine the role of dry minor mergers in elliptical galaxy formation.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 195
Copyright
Copyright © International Astronomical Union 2007

References

Bell, E. F. 2004, ApJ 608, 752.CrossRefGoogle Scholar
Boylan-Kolchin, M., & Ma, C.-P. 2006, MNRAS submitted (astro-ph/0608122).Google Scholar
de Lucia, G., & Blaizot, J. 2006, MNRAS submitted (astro-ph/0606519).Google Scholar
Faber, S. M. 2006, ApJ submitted (astro-ph/0506044).Google Scholar
Taffoni, G., Mayer, L., Colpi, M., & Governato, F. 2003, MNRAS 341, 434.CrossRefGoogle Scholar
Tran, K.-V. H., van Dokkum, P., Franx, M., Illingworth, G. D., Kelson, D. D., & Förster Schreiber, N. M. 2005, ApJ 627, L25.CrossRefGoogle Scholar
Shen, S. 2003, MNRAS 343, 978.Google Scholar