Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:astro-ph/0612511)
· References in the article
· Citations to the Article (33) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (3)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
The Ages and Masses of Lyα Galaxies at z ~ 4.5
Authors:
Finkelstein, Steven L.; Rhoads, James E.; Malhotra, Sangeeta; Pirzkal, Norbert; Wang, Junxian
Affiliation:
AA(Department of Physics, Arizona State University, Tempe, AZ 85287.), AB(School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287.), AC(School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287.), AD(Space Telescope Science Institute, Baltimore, MD 21218.), AE(University of Science and Technology of China, Hefei, Anhui 230026, China.)
Publication:
The Astrophysical Journal, Volume 660, Issue 2, pp. 1023-1029. (ApJ Homepage)
Publication Date:
05/2007
Origin:
UCP
ApJ Keywords:
Galaxies: Evolution, Galaxies: Fundamental Parameters, Galaxies: High-Redshift, Galaxies: ISM
DOI:
10.1086/513462
Bibliographic Code:
2007ApJ...660.1023F

Abstract

We examine the stellar populations of a sample of 98 z~4.5 Lyα-emitting galaxies using their broadband colors derived from deep photometry at the Multiple Mirror Telescope (MMT). These galaxies were selected by narrowband excess from the Large Area Lyman Alpha survey. Twenty-two galaxies are detected in two or more of our MMT filters (g', r', i,' and z'), with calculated rest-frame equivalent widths (EWs) from 5 to 800 Å. By comparing broad- and narrowband colors of these galaxies to synthetic colors from stellar population models, we determine their ages and stellar masses. The highest EW objects have an average age of 4 Myr, consistent with ongoing star formation. The lowest EW objects show an age of 40-200 Myr, consistent with the expectation that larger numbers of older stars are causing low EWs. We found masses ranging from 2×107 Msolar for the youngest objects in the sample to 2×109 Msolar for the oldest. It is possible that dust effects could produce large EWs even in older populations by allowing the Lyα photons to escape, even while the continuum is extinguished, and we present models for this scenario also.

Observations reported here were obtained at the MMT Observatory, a joint facility of the University of Arizona and the Smithsonian Institution.


Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints