Gas properties in emission-line galaxies

DOI

With the aim of distinguishing between possible physical mechanisms acting on galaxies when they fall into clusters, we study the properties of the gas and the stars in a sample of 422 emission-line galaxies from the European Southern Observatory Distant Cluster Survey in different environments up to z~1. We identify galaxies with kinematical disturbances (from emission lines in their 2D spectra) and find that they are more frequent in clusters than in the field.

Cone search capability for table J/MNRAS/417/1996/tablea1 (Measured rotation velocities and emission scalelengths)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74171996
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/417/1996
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/417/1996
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/417/1996
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/417/1996
Provenance
Creator Jaffe Y.L.; Aragon-Salamanca A.; Kuntschner H.; Bamford S.; Hoyos C.,De Lucia G.; Halliday C.; Milvang-Jensen B.; Poggianti B.; Rudnick G.,Saglia R.P.; Sanchez-Blazquez P.; Zaritsky D.
Publisher CDS
Publication Year 2012
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; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics