YSO candidates in the IR dust bubble N6

DOI

We have carried out a multiwavelength study of the infrared dust bubble N6 to extensively investigate the molecular environs and star-forming activities therein. 99 young stellar objects (YSOs) have been identified based on their infrared colors. A group of YSOs reside inside the ring, indicating active star formation in N6. Although no confirmative features of triggered star formation are detected, the bubble and the enclosed HII region have profoundly reconstructed the natal cloud and altered the dynamics therein.

Cone search capability for table J/ApJ/797/40/table56 (Magnitudes and model parameters of YSO candidates (tables 5 and 6 of the paper))

Identifier
DOI http://doi.org/10.26093/cds/vizier.17970040
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/797/40
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/797/40
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/797/40
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/797/40
Provenance
Creator Yuan J.-H.; Wu Y.; Li J.Z.; Liu H.
Publisher CDS
Publication Year 2017
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; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy