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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S256(4), p. 184-188, 2008

DOI: 10.1017/s1743921308028433

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Early results from the SAGE-SMC Spitzer legacy

Journal article published in 2008 by Karl D. Gordon ORCID, M. Meixner, R. D. Blum, W. Reach ORCID, B. A. Whitney, J. Harris, R. Indebetouw, A. D. Bolatto, J.-P. Bernard, M. Sewilo, B. L. Babler ORCID, M. Block, C. Bot ORCID, S. Bracker, L. Carlson and other authors.
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractEarly results from the SAGE-SMC (Surveying the Agents of Galaxy Evolution in the tidally-disrupted, low-metallicity Small Magellanic Cloud) Spitzer legacy program are presented. These early results concentrate on the SAGE-SMC MIPS observations of the SMC Tail region. This region is the high H i column density portion of the Magellanic Bridge adjacent to the SMC Wing. We detect infrared dust emission and measure the gas-to-dust ratio in the SMC Tail and find it similar to that of the SMC Body. In addition, we find two embedded cluster regions that are resolved into multiple sources at all MIPS wavelengths.

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