Kinematics across the Hubble sequence Virtual Observatory Resource

Authors

1. Ho L.C.

Published by

CDS

Abstract

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.

Keywords

1. galaxies
2. catalogs
3. h-i-line-emission
4. galaxy-kinematics
5. galaxy-classification-systems

Bibliographic source Bibcode

2007ApJ...668...94H

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/668/94

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/668/94

Document Object Identifer DOI

doi:10.26093/cds/vizier.16680094

Access

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https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/668/94
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/668/94
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/668/94

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For use with a cone search client (e.g., TOPCAT).
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https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/668/94/sample?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/668/94/sample?