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Young Stellar Objects in the Low-Metallicity Small Magellanic Cloud

Published online by Cambridge University Press:  21 March 2013

M. Sewiło
Affiliation:
The Johns Hopkins University, Baltimore, MD, USA, email: msewilo@pha.jhu.edu
L. R. Carlson
Affiliation:
Leiden Observatory, Leiden, The Netherlands
J. P. Seale
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA
R. Indebetouw
Affiliation:
University of Virginia, Charlottesville, VA, USA
M. Meixner
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA
B. A. Whitney
Affiliation:
Space Science Institute, Boulder, CO, USA
T. R. Robitaille
Affiliation:
Max Planck Institute for Astronomy, Heidelberg, Germany
J. M. Oliveira
Affiliation:
Keele University, Keele, UK
K. Gordon
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA
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Abstract

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The Spitzer Legacy Program “Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low-Metallicity Small Magellanic Cloud” (SAGE-SMC; Gordon et al. 2011) allows a global study of star formation in the SMC at high enough resolution to resolve individual cores and protostars at a range of mid-IR wavelengths. Using the SAGE-SMC IRAC (3.6 - 8.0 μm) and MIPS (24 and 70 μm) catalogs and images combined with the near-IR and optical data, we identified a population of ∼1100 intermediate- to high-mass Young Stellar Objects (YSOs) in the SMC (3 × more than previously known). We investigate the properties of the YSOs and how they relate to the galaxy's structure and gas and dust distribution.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

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