Hostname: page-component-76fb5796d-2lccl Total loading time: 0 Render date: 2024-04-26T11:31:44.083Z Has data issue: false hasContentIssue false
  • English
  • Français

Morphologies and Substructures of UV Star-Forming Galaxies at Intermediate-z

Published online by Cambridge University Press:  21 March 2013

E. N. Voyer ,
D. F. de Mello ,
S. M. Blevins ,
H. I. Teplitz ,
J. P. Gardner ,
B. D. Siana  and
E. Soto
E. N. Voyer
Affiliation:
Aix Marseille Université, CNRS, LAM, UMR 7326, 13388 Marseille, France The Catholic University of America, Physics Department, Washington, DC 20064, USA
D. F. de Mello
Affiliation:
The Catholic University of America, Physics Department, Washington, DC 20064, USA Observational Cosmology Laboratory, Code 665, NASA's GSFC, Greenbelt, MD 20771, USA
S. M. Blevins
Affiliation:
The Catholic University of America, Physics Department, Washington, DC 20064, USA
H. I. Teplitz
Affiliation:
Infrared Processing and Analysis Center, Caltech, Pasadena, CA 91125, USA
J. P. Gardner
Affiliation:
Observational Cosmology Laboratory, Code 665, NASA's GSFC, Greenbelt, MD 20771, USA
B. D. Siana
Affiliation:
Department of Physics and Astronomy, University of California, Riverside, CA 92521, USA
E. Soto
Affiliation:
The Catholic University of America, Physics Department, Washington, DC 20064, USA
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.

Exploring potential links between the internal physical processes of galaxies with respect to their external morphologies can reveal connections between past and present populations. One primary physical driver of galaxy evolution is star formation, which is directly detected from UV emission. Here, we summarize a study investigating the optical and UV morphologies of rest-frame UV-detected star-forming galaxies at intermediate redshifts (0.1<z<1.2) observed with the Hubble Space Telescope (HST) Solar Blind Channel (far-UV) and Wide Field PlanetaryCamera 2 (WFPC2; U-band) in the Great Observatories Origins Deep Survey fields.

Keywords

ultraviolet: galaxies — galaxies: structure — galaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 194
Copyright
Copyright © International Astronomical Union 2013

References

Dahlen, T., Mobasher, B., Dickinson, M., et al. 2010 ApJ, 724, 425CrossRefGoogle Scholar
Elmegreen, B. G. & Elmegreen, D. M. 2005, ApJ, 627, 632Google Scholar
Teplitz, H. I., Siana, B., Brown, T. M., et al. 2006, AJ, 132, 853Google Scholar
Voyer, E. N., de Mello, D. F., Siana, B., et al. 2009, AJ, 138, 598Google Scholar
Voyer, E. N., Gardner, J. P., Teplitz, H. I., Siana, B. D., & de Mello, D. F. 2011, ApJ, 736, 80CrossRefGoogle Scholar