Galaxies with strong PAH emission Virtual Observatory Resource

Authors

1. Haas M.
2. Leipski C.
3. Siebenmorgen R.
4. Meusinger H.
5. Drass H.
6. Chini R.

Published by

CDS

Abstract

This is the fourth in a series of papers based on the ISOCAM Parallel Survey at 6.7um. While the first three papers have been devoted to active galactic nuclei (AGN), here we report on emission-line galaxies without AGN signatures in their optical spectra. Polycyclic aromatic hydrocarbon (PAH) emission has been found in both starbursts and modestly starforming galaxies, but the relation between starforming activity and PAH luminosity is still a matter of debate. The different correlation degrees could be caused by the variety of optical and far-infrared sample selection criteria. In order to obtain a census of the typical properties of PAH emitting galaxies, we here study moderately distant galaxies which have been selected by their PAH emission.

Keywords

1. Galaxies
2. Infrared sources
3. Infrared photometry
4. Interstellar medium

Bibliographic source Bibcode

2009A&A...507..713H

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/507/713

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/507/713

Document Object Identifer DOI

doi:10.26093/cds/vizier.35070713

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/507/713
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/507/713
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/507/713

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/A+A/507/713/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/507/713/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/507/713/table1?