Early results from the SAGE-SMC Spitzer legacy

Karl D. Gordon, M. Meixner, R. D. Blum, W. Reach, B. A. Whitney, J. Harris, R. Indebetouw, A. D. Bolatto, J. P. Bernard, M. Sewilo, B. L. Babler, M. Block, C. Bot, S. Bracker, L. Carlson, E. Churchwell, G. C. Clayton, M. Cohen, C. W. Engelbracht, Y. FukuiV. Gorjian, S. Hony, J. L. Hora, F. Israel, A. Kawamura, A. K. Leroy, A. Li, S. Madden, A. R. Marble, F. Markwick-Kemper, M. Meade, K. A. Misselt, A. Mizuno, N. Mizuno, E. Muller, J. M. Oliveira, K. Olsen, T. Onishi, R. Paladini, D. Paradis, S. Points, T. Robitaille, D. Rubin, K. M. Sandstrom, S. Sato, H. Shibai, J. D. Simon, L. J. Smith, S. Srinivasan, A. G G M Tielens, U. P. Vijh, S. Van Dyk, J. Th Van Loon, K. Volk, Dennis F Zaritsky

Research output: Contribution to journalArticle

Abstract

Early 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.

Original languageEnglish (US)
Pages (from-to)184-188
Number of pages5
JournalProceedings of the International Astronomical Union
Volume4
Issue numberS256
DOIs
StatePublished - Jul 2008
Externally publishedYes

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dust
Magellanic clouds
wings
surveying
metallicity
galaxies
wavelength
gases
gas
wavelengths
programme

Keywords

  • Galaxies: individual (SMC)
  • Galaxies: ISM
  • Infrared: ISM
  • Magellanic Clouds

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

Gordon, K. D., Meixner, M., Blum, R. D., Reach, W., Whitney, B. A., Harris, J., ... Zaritsky, D. F. (2008). Early results from the SAGE-SMC Spitzer legacy. Proceedings of the International Astronomical Union, 4(S256), 184-188. https://doi.org/10.1017/S1743921308028433

Early results from the SAGE-SMC Spitzer legacy. / Gordon, Karl D.; Meixner, M.; Blum, R. D.; Reach, W.; Whitney, B. A.; Harris, J.; Indebetouw, R.; Bolatto, A. D.; Bernard, J. P.; Sewilo, M.; Babler, B. L.; Block, M.; Bot, C.; Bracker, S.; Carlson, L.; Churchwell, E.; Clayton, G. C.; Cohen, M.; Engelbracht, C. W.; Fukui, Y.; Gorjian, V.; Hony, S.; Hora, J. L.; Israel, F.; Kawamura, A.; Leroy, A. K.; Li, A.; Madden, S.; Marble, A. R.; Markwick-Kemper, F.; Meade, M.; Misselt, K. A.; Mizuno, A.; Mizuno, N.; Muller, E.; Oliveira, J. M.; Olsen, K.; Onishi, T.; Paladini, R.; Paradis, D.; Points, S.; Robitaille, T.; Rubin, D.; Sandstrom, K. M.; Sato, S.; Shibai, H.; Simon, J. D.; Smith, L. J.; Srinivasan, S.; Tielens, A. G G M; Vijh, U. P.; Van Dyk, S.; Van Loon, J. Th; Volk, K.; Zaritsky, Dennis F.

In: Proceedings of the International Astronomical Union, Vol. 4, No. S256, 07.2008, p. 184-188.

Research output: Contribution to journalArticle

Gordon, KD, Meixner, M, Blum, RD, Reach, W, Whitney, BA, Harris, J, Indebetouw, R, Bolatto, AD, Bernard, JP, Sewilo, M, Babler, BL, Block, M, Bot, C, Bracker, S, Carlson, L, Churchwell, E, Clayton, GC, Cohen, M, Engelbracht, CW, Fukui, Y, Gorjian, V, Hony, S, Hora, JL, Israel, F, Kawamura, A, Leroy, AK, Li, A, Madden, S, Marble, AR, Markwick-Kemper, F, Meade, M, Misselt, KA, Mizuno, A, Mizuno, N, Muller, E, Oliveira, JM, Olsen, K, Onishi, T, Paladini, R, Paradis, D, Points, S, Robitaille, T, Rubin, D, Sandstrom, KM, Sato, S, Shibai, H, Simon, JD, Smith, LJ, Srinivasan, S, Tielens, AGGM, Vijh, UP, Van Dyk, S, Van Loon, JT, Volk, K & Zaritsky, DF 2008, 'Early results from the SAGE-SMC Spitzer legacy', Proceedings of the International Astronomical Union, vol. 4, no. S256, pp. 184-188. https://doi.org/10.1017/S1743921308028433
Gordon KD, Meixner M, Blum RD, Reach W, Whitney BA, Harris J et al. Early results from the SAGE-SMC Spitzer legacy. Proceedings of the International Astronomical Union. 2008 Jul;4(S256):184-188. https://doi.org/10.1017/S1743921308028433
Gordon, Karl D. ; Meixner, M. ; Blum, R. D. ; Reach, W. ; Whitney, B. A. ; Harris, J. ; Indebetouw, R. ; Bolatto, A. D. ; Bernard, J. P. ; Sewilo, M. ; Babler, B. L. ; Block, M. ; Bot, C. ; Bracker, S. ; Carlson, L. ; Churchwell, E. ; Clayton, G. C. ; Cohen, M. ; Engelbracht, C. W. ; Fukui, Y. ; Gorjian, V. ; Hony, S. ; Hora, J. L. ; Israel, F. ; Kawamura, A. ; Leroy, A. K. ; Li, A. ; Madden, S. ; Marble, A. R. ; Markwick-Kemper, F. ; Meade, M. ; Misselt, K. A. ; Mizuno, A. ; Mizuno, N. ; Muller, E. ; Oliveira, J. M. ; Olsen, K. ; Onishi, T. ; Paladini, R. ; Paradis, D. ; Points, S. ; Robitaille, T. ; Rubin, D. ; Sandstrom, K. M. ; Sato, S. ; Shibai, H. ; Simon, J. D. ; Smith, L. J. ; Srinivasan, S. ; Tielens, A. G G M ; Vijh, U. P. ; Van Dyk, S. ; Van Loon, J. Th ; Volk, K. ; Zaritsky, Dennis F. / Early results from the SAGE-SMC Spitzer legacy. In: Proceedings of the International Astronomical Union. 2008 ; Vol. 4, No. S256. pp. 184-188.
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abstract = "Early 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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T1 - Early results from the SAGE-SMC Spitzer legacy

AU - Gordon, Karl D.

AU - Meixner, M.

AU - Blum, R. D.

AU - Reach, W.

AU - Whitney, B. A.

AU - Harris, J.

AU - Indebetouw, R.

AU - Bolatto, A. D.

AU - Bernard, J. P.

AU - Sewilo, M.

AU - Babler, B. L.

AU - Block, M.

AU - Bot, C.

AU - Bracker, S.

AU - Carlson, L.

AU - Churchwell, E.

AU - Clayton, G. C.

AU - Cohen, M.

AU - Engelbracht, C. W.

AU - Fukui, Y.

AU - Gorjian, V.

AU - Hony, S.

AU - Hora, J. L.

AU - Israel, F.

AU - Kawamura, A.

AU - Leroy, A. K.

AU - Li, A.

AU - Madden, S.

AU - Marble, A. R.

AU - Markwick-Kemper, F.

AU - Meade, M.

AU - Misselt, K. A.

AU - Mizuno, A.

AU - Mizuno, N.

AU - Muller, E.

AU - Oliveira, J. M.

AU - Olsen, K.

AU - Onishi, T.

AU - Paladini, R.

AU - Paradis, D.

AU - Points, S.

AU - Robitaille, T.

AU - Rubin, D.

AU - Sandstrom, K. M.

AU - Sato, S.

AU - Shibai, H.

AU - Simon, J. D.

AU - Smith, L. J.

AU - Srinivasan, S.

AU - Tielens, A. G G M

AU - Vijh, U. P.

AU - Van Dyk, S.

AU - Van Loon, J. Th

AU - Volk, K.

AU - Zaritsky, Dennis F

PY - 2008/7

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AB - Early 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.

KW - Galaxies: individual (SMC)

KW - Galaxies: ISM

KW - Infrared: ISM

KW - Magellanic Clouds

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