YSOs in the l=+45 ISOGAL field Virtual Observatory Resource

Authors

1. Felli M.
2. Comoretto G.
3. Testi L.
4. Omont A.
5. Schuller F.

Published by

CDS

Abstract

The 7 and 15{mu}m observations of the Galaxy obtained by the ISOGAL program offer an unique possibility to investigate and separate the different populations of stars in the Galactic Plane, in particular to study the population of low flux density YSOs which could not be detected with IRAS.

Keywords

1. young-stellar-objects
2. infrared-sources
3. infrared-photometry

Bibliographic source Bibcode

2000A&A...362..199F

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/362/199

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/362/199

Document Object Identifer DOI

doi:10.26093/cds/vizier.33620199

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/362/199
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/362/199
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/362/199

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/362/199/table4?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/362/199/table4?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/362/199/table4?