Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-28T16:10:13.331Z Has data issue: false hasContentIssue false

Young Star Clusters in the Small Magellanic Cloud: Impact of Local and Global Conditions on Star Formation

Published online by Cambridge University Press:  01 June 2008

Elena Sabbi
Affiliation:
Space Telescope Science Institute3700 San Martin Drive, Baltimore, MD, 21218, USA email: sabbi@stsci.edu
Linda J. Smith
Affiliation:
Space Telescope Science Institute3700 San Martin Drive, Baltimore, MD, 21218, USA email: sabbi@stsci.edu University College LondonLondon, UK
Lynn R. Carlson
Affiliation:
Johns Hopkins UniversityBaltimore, MD, USA
Antonella Nota
Affiliation:
Space Telescope Science Institute3700 San Martin Drive, Baltimore, MD, 21218, USA email: sabbi@stsci.edu European Space Agency, Research and Scientific Support DepartmentBaltimore, MD, USA
Monca Tosi
Affiliation:
INAF-Osservatorio Astronomico di BolognaBologna, Italy
Michele Cignoni
Affiliation:
INAF-Osservatorio Astronomico di BolognaBologna, Italy
Jay S. Gallagher III
Affiliation:
University of WisconsinMadison, WI, USA
Marco Sirianni
Affiliation:
Space Telescope Science Institute3700 San Martin Drive, Baltimore, MD, 21218, USA email: sabbi@stsci.edu European Space Agency, Research and Scientific Support DepartmentBaltimore, MD, USA
Margaret Meixner
Affiliation:
Space Telescope Science Institute3700 San Martin Drive, Baltimore, MD, 21218, USA email: sabbi@stsci.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We compared deep images acquired with the Advanced Camera for Surveys on board of the Hubble Space Telescope with mid-IR Spitzer Space Telescope images and University College London Echelle Spectrograph spectra of NGC 346 and NGC 602, two of the youngest star clusters in the Small Magellanic Cloud. Our multi-wavelength approach allowed us to infer very different origins for the clusters: while NGC 346 is likely the result of the hierarchical collapse of a giant molecular cloud, NGC 602 is probably the result of the collision and consequent interaction of two H I shells of gas.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Bonnell, I. A. & Bate, M. R. 2002, MNRAS, 336, 659CrossRefGoogle Scholar
Bonnell, I. A., Bate, M. R., & Vine, S. G. 2003, MNRAS, 343, 413CrossRefGoogle Scholar
Cignoni, M. et al. 2008, Proceedings IAU Symposium No. 255, “Low-Metallicity Star Formation: From the Firts Stars to Dwarf Galaxies”, Hunt, L.K., Madden, S., & Schneider, R., eds.Google Scholar
Cignoni, M. et al. 2008, AJ, (submitted)Google Scholar
Klessen, R. S. & Burkert, A. 2000, ApJS, 128, 287CrossRefGoogle Scholar
Mokiem, M. R., et al. 2007, A&A, 473, 603Google Scholar
Nigra, L., Gallagher, J. S. III, Smith, L. J., Stanimirović, S., Nota, A., & Sabbi, E. 2008, PASP, (accepted for publication) astro-ph/0808.1033Google Scholar
Nota, A. et al. 2006, ApJ, 640, L29CrossRefGoogle Scholar
Ostriker, E. C., Stone, J. M., & Gammie, C. F. 2001, ApJ, 546, 980CrossRefGoogle Scholar
Rubio, et al. 2000, A&AGoogle Scholar
Sabbi, E., Sirianni, M., Nota, A., Tosi, M., Gallagher, J., Meixner, M., Oey, M. S., Walterbos, R., Pasquali, A., Smith, L.J., & Angeretti, L. 2007, AJ, 133, 44CrossRefGoogle Scholar
Sabbi, E., Sirianni, M., Nota, A., TOsi, M., Gallagher, J., Smith, L. J., Angeretti, L., Oey, M. S., Walterbos, R., & Pasquali, A. 2008, AJ, 135, 173CrossRefGoogle Scholar
Simon, J. H., et al. 2007, ApJ, 670, 313CrossRefGoogle Scholar
Stanimirović, S., Staveley-Smith, L., Dickey, J. M., Sault, R. J., & Snowden, S. L. 1999, MNRAS, 302, 417CrossRefGoogle Scholar
Staveley-Smith, L., Sault, R. J., Hatzidimitriou, D., Kesteven, M. J., & McConnell, D. 1997, MNRAS, 289, 225CrossRefGoogle Scholar