YSOs in the l=+45 ISOGAL field

DOI

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.

Cone search capability for table J/A+A/362/199/table4 (List of sources that satisfy the confidence criteria mag(7um)<=9.5 and mag(15um)<=8, or are classified as cYSO (candidate YSOs))

Identifier
DOI http://doi.org/10.26093/cds/vizier.33620199
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/362/199
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/362/199
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/362/199
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/362/199
Provenance
Creator Felli M.; Comoretto G.; Testi L.; Omont A.; Schuller F.
Publisher CDS
Publication Year 2000
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy