H_2_/HI ratio in galaxies Virtual Observatory Resource

Authors
  1. Obreschkow D.
  2. Rawlings S.
  3. Published by
    CDS
Abstract

We revisit the mass ratio {eta}_galaxy_ between molecular hydrogen (H2) and atomic hydrogen (HI) in different galaxies from a phenomenological and theoretical viewpoint.

Keywords
  1. Radio galaxies
  2. H I line emission
  3. Radio astronomy
Bibliographic source Bibcode
2009MNRAS.394.1857O
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/394/1857
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/394/1857

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/394/1857
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/394/1857
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/394/1857
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/394/1857/tablea1?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/394/1857/tablea1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/394/1857/tablea1?

History

2009-11-09T14:31:37Z
Resource record created
2009-11-09T14:31:37Z
Created
2018-01-02T13:43:03Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr