S3MC: YSOs in N66, in SMC

DOI

We use Spitzer Space Telescope observations from the Spitzer Survey of the Small Magellanic Cloud (S^3^MC) to study the young stellar content of N66, the largest and brightest HII region in the SMC. In addition to large numbers of normal stars, we detect a significant population of bright, red infrared sources that we identify as likely to be young stellar objects (YSOs). We use spectral energy distribution (SED) fits to classify objects as ordinary (main-sequence or red giant) stars, asymptotic giant branch stars, background galaxies, and YSOs.

Cone search capability for table J/ApJ/669/327/table1 (Young Stellar Objects in N66)

Identifier
DOI http://doi.org/10.26093/cds/vizier.16690327
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/669/327
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/669/327
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/669/327
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/669/327
Provenance
Creator Simon J.D.; Bolatto A.D.; Whitney B.A.; Robitaille T.P.; Shah R.Y.,Makovoz D.; Stanimirovic S.; Barba R.H.; Rubio M.
Publisher CDS
Publication Year 2010
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; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy