YSO candidates in the IR dust bubble N6 Virtual Observatory Resource

Authors
  1. Yuan J.-H.
  2. Wu Y.
  3. Li J.Z.
  4. Liu H.
  5. Published by
    CDS
Abstract

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.

Keywords
  1. young-stellar-objects
  2. infrared-photometry
  3. stellar-masses
  4. effective-temperature
Bibliographic source Bibcode
2014ApJ...797...40Y
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/797/40
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/797/40
Document Object Identifer DOI
doi:10.26093/cds/vizier.17970040

Access

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https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/797/40
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/797/40
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/797/40
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https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/797/40/table56?
https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/797/40/table56?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/797/40/table56?

History

2017-01-02T11:39:04Z
Resource record created
2017-01-02T11:39:04Z
Created
2017-08-29T07:09:00Z
Updated

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