Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-14T17:09:50.310Z Has data issue: false hasContentIssue false
  • English
  • Français

The Secret Life of Galaxies

Published online by Cambridge University Press:  10 April 2015

Alan Dressler  and
Louis Abramson
Alan Dressler
Affiliation:
The Observatories of the Carnegie Institution of Science, 813 Santa Barbara Street, Pasadena, CA 91101-1232, USA. email: dressler@obs.carnegiescience.edu
Louis Abramson
Affiliation:
Department of Astronomy & Astrophysics and Kavli Institute for Cosmological Physics, The University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA. email: labramson@uchicago.edu
Rights & Permissions [Opens in a new window]

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 have learned much about galaxy evolution since z = 2, and something to even higher redshifts. How can it be that we know so little about! the star formation histories (SFHs) of individual galaxies? Although great progress has been made accumulating huge samples with only rudimentary properties, progress in galaxy evolution means connecting what we've learned to detailed measurements of the life-histories of specific –- not just representative –- systems.

Keywords

galaxies: evolution - galaxies: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S311: Galaxy Masses as Constraints of Formation Models , July 2014 , pp. 140 - 145
Copyright
Copyright © International Astronomical Union 2015 

References

Abramson, L. E., Dressler, A., Gladders, M. D., et al. 2013, ApJ, 777, 124CrossRefGoogle Scholar
Abramson, L. E., Gladders, M. G., & Dressler, A., et al., 2014, in preparation.Google Scholar
Baade, W. 1958, Ricerche Astronomiche, 5, 3Google Scholar
Behroozi, P. S., Wechsler, R. H., & Conroy, C. 2013a, ApJ, 770, 57CrossRefGoogle Scholar
Behroozi, P. S., Marchesini, D., Wechsler, R. H., et al. 2013b, ApJ, 777, L10CrossRefGoogle Scholar
Dressler, A., Oemler, A., Jr., Poggianti, B. M., et al. 2013, ApJ, 770, 62CrossRefGoogle Scholar
Gladders, M. D., Oemler, A., Dressler, A., et al. 2013, ApJ, 770, 64CrossRefGoogle Scholar
Kelson, D. D. 2014, arXiv:1406.5191Google Scholar
Noeske, K. G., Weiner, B. J., Faber, S. M., et al. 2007, ApJ, 660, L43CrossRefGoogle Scholar
Oemler, A. Jr., Dressler, A., Gladders, M. G., et al. 2013, ApJ, 770, 63CrossRefGoogle Scholar
Oemler, A. Jr., Abramson, L. E., Gladders, M. G., et al., 2014, in preparation.Google Scholar
Madau, P. & Dickinson, M. 2014, ARA&A, 52, 415Google Scholar
Peng, Y.-j., Lilly, S. J., Kovač, K., et al. 2010, ApJ, 721, 193CrossRefGoogle Scholar
Poggianti, B. M., Smail, I., Dressler, A., et al. 1999, ApJ, 518, 576CrossRefGoogle Scholar
Simard, L., Mendel, J. T., Patton, D. R., Ellison, S. L., & McConnachie, A. W. 2011, ApJS, 196, 11CrossRefGoogle Scholar
Schawinski, K., Urry, C. M., Simmons, B. D., et al. 2014, MNRAS, 440, 889CrossRefGoogle Scholar
Simha, V., Weinberg, D. H., Conroy, C., et al. 2014, arXiv:1404.0402Google Scholar
Tomczak, A. R., Quadri, R. F., Tran, K.-V. H., et al. 2014, ApJ, 783, 85CrossRefGoogle Scholar
Vulcani, B., Poggianti, B. M., Fritz, J., et al., 2014, submitted to ApJ. Abramson, L. E., Gladders, M. G., et al., 2014, in preparation.Google Scholar
Whitaker, K. E., van Dokkum, P. G., Brammer, G., & Franx, M. 2012, ApJ, 754, L29CrossRefGoogle Scholar