The dynamical masses, densities, and star formation scaling relations of Lyα galaxies
Abstract
We present the first dynamical mass measurements for Lyα galaxies at high redshift, based on velocity dispersion measurements from rest-frame optical emission lines and size measurements from Hubble Space Telescope imaging, for nine galaxies drawn from four surveys. We use these measurements to study Lyα galaxies in the context of galaxy scaling relations. The resulting dynamical masses range from 10{sup 9} to 10{sup 10} M {sub ☉}. We also fit stellar population models to our sample and use them to place the Lyα sample on a stellar mass versus line width relation. The Lyα galaxies generally follow the same scaling relation as star-forming galaxies at lower redshift, although, lower stellar mass fits are also acceptable in ∼1/3 of the Lyα galaxies. Using the dynamical masses as an upper limit on gas mass, we show that Lyα galaxies have unusually active star formation for their gas mass surface density. This behavior is consistent with what is observed in starburst galaxies, despite the typically smaller masses and sizes of the Lyα galaxy population. Finally, we examine the mass densities of these galaxies and show that their future evolution likely requires dissipational ('wet') merging. In short, we find that Lyα galaxies are low-massmore »
- Authors:
-
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287 (United States)
- Department of Astronomy, University of Texas at Austin, 1 University Station C1400, Austin, TX 78712 (United States)
- DARK Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø (Denmark)
- Publication Date:
- OSTI Identifier:
- 22348355
- Resource Type:
- Journal Article
- Journal Name:
- Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 780; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; DENSITY; DISPERSIONS; EMISSION; EVOLUTION; GALAXIES; LINE WIDTHS; MASS; RED SHIFT; SPACE; STARS; SURFACES; TELESCOPES; VELOCITY
Citation Formats
Rhoads, James E., Malhotra, Sangeeta, Richardson, Mark L. A., McLinden, Emily M., Finkelstein, Steven L., Fynbo, Johan P. U., and Tilvi, Vithal S., E-mail: James.Rhoads@asu.edu. The dynamical masses, densities, and star formation scaling relations of Lyα galaxies. United States: N. p., 2014.
Web. doi:10.1088/0004-637X/780/1/20.
Rhoads, James E., Malhotra, Sangeeta, Richardson, Mark L. A., McLinden, Emily M., Finkelstein, Steven L., Fynbo, Johan P. U., & Tilvi, Vithal S., E-mail: James.Rhoads@asu.edu. The dynamical masses, densities, and star formation scaling relations of Lyα galaxies. United States. https://doi.org/10.1088/0004-637X/780/1/20
Rhoads, James E., Malhotra, Sangeeta, Richardson, Mark L. A., McLinden, Emily M., Finkelstein, Steven L., Fynbo, Johan P. U., and Tilvi, Vithal S., E-mail: James.Rhoads@asu.edu. 2014.
"The dynamical masses, densities, and star formation scaling relations of Lyα galaxies". United States. https://doi.org/10.1088/0004-637X/780/1/20.
@article{osti_22348355,
title = {The dynamical masses, densities, and star formation scaling relations of Lyα galaxies},
author = {Rhoads, James E. and Malhotra, Sangeeta and Richardson, Mark L. A. and McLinden, Emily M. and Finkelstein, Steven L. and Fynbo, Johan P. U. and Tilvi, Vithal S., E-mail: James.Rhoads@asu.edu},
abstractNote = {We present the first dynamical mass measurements for Lyα galaxies at high redshift, based on velocity dispersion measurements from rest-frame optical emission lines and size measurements from Hubble Space Telescope imaging, for nine galaxies drawn from four surveys. We use these measurements to study Lyα galaxies in the context of galaxy scaling relations. The resulting dynamical masses range from 10{sup 9} to 10{sup 10} M {sub ☉}. We also fit stellar population models to our sample and use them to place the Lyα sample on a stellar mass versus line width relation. The Lyα galaxies generally follow the same scaling relation as star-forming galaxies at lower redshift, although, lower stellar mass fits are also acceptable in ∼1/3 of the Lyα galaxies. Using the dynamical masses as an upper limit on gas mass, we show that Lyα galaxies have unusually active star formation for their gas mass surface density. This behavior is consistent with what is observed in starburst galaxies, despite the typically smaller masses and sizes of the Lyα galaxy population. Finally, we examine the mass densities of these galaxies and show that their future evolution likely requires dissipational ('wet') merging. In short, we find that Lyα galaxies are low-mass cousins of larger starbursts.},
doi = {10.1088/0004-637X/780/1/20},
url = {https://www.osti.gov/biblio/22348355},
journal = {Astrophysical Journal},
issn = {0004-637X},
number = 1,
volume = 780,
place = {United States},
year = {Wed Jan 01 00:00:00 EST 2014},
month = {Wed Jan 01 00:00:00 EST 2014}
}