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The Astrophysical journal, 2009-04, Vol.695 (1), p.L67-L71
2009

Details

Autor(en) / Beteiligte
Titel
A Population of Metal-Poor Galaxies with ~L Luminosities at Intermediate Redshifts
Ist Teil von
  • The Astrophysical journal, 2009-04, Vol.695 (1), p.L67-L71
Ort / Verlag
IOP Publishing
Erscheinungsjahr
2009
Link zum Volltext
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
  • We present new spectroscopy and metallicity estimates for a sample of 15 star-forming galaxies with redshifts in the range 0.29-0.42. These objects were selected in the KPNO International Spectroscopic Survey via their strong emission lines seen in red objective-prism spectra. Originally thought to be intermediate-redshift Seyfert 2 galaxies, our new spectroscopy in the far red has revealed these objects to be metal-poor star-forming galaxies. These galaxies follow a luminosity-metallicity (L - Z) relation that parallels the one defined by low-redshift galaxies, but is offset by a factor of more than 10 to lower abundances. The amount of chemical and/or luminosity evolution required to place these galaxies on the local L-Z relation is extreme, suggesting that these galaxies are in a very special stage of their evolution. They may be late-forming massive systems, which would challenge the current paradigm of galaxy formation. Alternatively, they may represent intense starbursts in dwarf-dwarf mergers or a major infall episode of pristine gas into a pre-existing galaxy. In any case, these objects represent an extreme stage of galaxy evolution taking place at relatively low redshift.
Sprache
Englisch
Identifikatoren
ISSN: 1538-4357, 0004-637X
eISSN: 1538-4357
DOI: 10.1088/0004-637X/695/1/L67
Titel-ID: cdi_proquest_miscellaneous_20553315
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