Kinematics across the Hubble sequence

DOI

The correlation between the maximum rotational velocity of the disk (vm) and the central stellar velocity dispersion of the bulge (sigma0) offers insights into the relationship between the halo and the bulge. We have assembled integrated HI line widths and central stellar velocity dispersions to study the vm-sigma0 relation for 792 galaxies spanning a broad range of Hubble types.

Cone search capability for table J/ApJ/668/94/sample (The sample of galaxies and their kinematical data)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16680094
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/668/94
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/668/94
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/668/94
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/668/94
Provenance
Creator Ho L.C.
Publisher CDS
Publication Year 2010
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; Interstellar medium; Natural Sciences; Observational Astronomy; Physics