LAE Galaxies at High Redshift: Formation Sites for Low-Metal Globular Clusters

Bruce G. Elmegreen, Sangeeta Malhotra, James Rhoads

Research output: Contribution to journalArticle

Abstract

Lyman-α emitting (LAE) galaxies observed at intermediate to high redshift have the correct size, mass, star formation rate, metallicity, and space density to have been the formation sites of metal-poor globular clusters. LAEs are typically small galaxies with transient starbursts. They should accrete onto spiral and elliptical galaxies over time, delivering metal-poor clusters into the larger galaxies' halos as they themselves get dispersed by tidal forces. The galaxy WLM is a good example of a dwarf remnant from a very early starburst that contains a metal-poor globular cluster but failed to get incorporated into the Milky Way or M31 because of its remote location in the local group.

Original languageEnglish (US)
Pages (from-to)257-258
Number of pages2
JournalProceedings of the International Astronomical Union
Volume10
Issue numberH16
DOIs
StatePublished - 2012

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globular clusters
galaxies
metal
metals
space density
elliptical galaxies
metal clusters
spiral galaxies
star formation rate
metallicity
halos

Keywords

  • galaxies: dwarf
  • galaxies: high-redshift
  • galaxies: star clusters
  • globular clusters: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

LAE Galaxies at High Redshift : Formation Sites for Low-Metal Globular Clusters. / Elmegreen, Bruce G.; Malhotra, Sangeeta; Rhoads, James.

In: Proceedings of the International Astronomical Union, Vol. 10, No. H16, 2012, p. 257-258.

Research output: Contribution to journalArticle

Elmegreen, Bruce G. ; Malhotra, Sangeeta ; Rhoads, James. / LAE Galaxies at High Redshift : Formation Sites for Low-Metal Globular Clusters. In: Proceedings of the International Astronomical Union. 2012 ; Vol. 10, No. H16. pp. 257-258.
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