Far infrared Seyfert galaxies Virtual Observatory Resource

Authors
  1. Liu Y.-L.
  2. Published by
    CDS
Abstract

Confusing sources of Seyfert and HII galaxies in IRAS point source catalogue may be caused by companion objects of those galaxies. Comparison between confused galaxies and non-confused galaxies have been made. The preliminary comparison shows that confused galaxies are fainter than nonconfused galaxies generally, and colour diagrams illustrate that confused Seyferts are separated from nonconfused Seyferts obviously.

Keywords
  1. seyfert-galaxies
  2. galaxies
  3. infrared-sources
Bibliographic source Bibcode
1991PBeiO..18....7L
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/PBeiO/18.7
IVOA Identifier IVOID
ivo://CDS.VizieR/J/other/PBeiO/18.7

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/PBeiO/18.7
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/PBeiO/18.7
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/PBeiO/18.7
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

1998-02-24T17:27:05Z
Resource record created
1998-02-24T16:27:15Z
Updated
1998-02-24T17:27:05Z
Created

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