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. Fukui; V. 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; D. Zaritsky

doi:10.1017/S1743921308028433

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, D. Zaritsky

Astronomy

Research output: Contribution to journal › Article › peer-review

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 language	English (US)
Pages (from-to)	184-188
Number of pages	5
Journal	Proceedings of the International Astronomical Union
Volume	4
Issue number	S256
DOIs	https://doi.org/10.1017/S1743921308028433
State	Published - Jul 2008

Keywords

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

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1017/S1743921308028433

Cite this

Gordon, K. 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., ... Zaritsky, D. (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

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, D 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

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title = "Early results from the SAGE-SMC Spitzer legacy",

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.",

keywords = "Galaxies: ISM, Galaxies: individual (SMC), Infrared: ISM, Magellanic Clouds",

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

year = "2008",

month = jul,

doi = "10.1017/S1743921308028433",

language = "English (US)",

volume = "4",

pages = "184--188",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

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TY - JOUR

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, D.

PY - 2008/7

Y1 - 2008/7

N2 - 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.

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: ISM

KW - Galaxies: individual (SMC)

KW - Infrared: ISM

KW - Magellanic Clouds

UR - http://www.scopus.com/inward/record.url?scp=84884893492&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84884893492&partnerID=8YFLogxK

U2 - 10.1017/S1743921308028433

DO - 10.1017/S1743921308028433

M3 - Article

AN - SCOPUS:84884893492

SN - 1743-9213

VL - 4

SP - 184

EP - 188

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - S256

ER -

Early results from the SAGE-SMC Spitzer legacy

Abstract

Keywords

ASJC Scopus subject areas

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