Chemical abundances in UV-selected galaxies

DOI

We discuss the chemical properties of a sample of UV-selected intermediate-redshift (0<=z<=0.4) galaxies in the context of their physical nature and star-formation history. This work represents an extension of our previous studies of the rest-frame UV-luminosity function (Treyer et al., 1998, Cat. ) and the star-formation properties of the same sample (Sullivan et al., 2000, Cat. ). We revisit the optical spectra of these galaxies and perform further emission-line measurements restricting the analysis to those spectra with the full set of emission lines required to derive chemical abundances. Our final sample consists of 68 galaxies with heavy-element abundance ratios and both UV and CCD B-band photometry.

Cone search capability for table J/MNRAS/330/75/table1 (The sample of UV-selected galaxies with measurements of chemical abundances (tables 1+2))

Identifier
DOI http://doi.org/10.26093/cds/vizier.73300075
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/330/75
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/330/75
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/330/75
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/330/75
Provenance
Creator Contini T.; Treyer M.A.; Sullivan M.; Ellis R.S.
Publisher CDS
Publication Year 2004
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics