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. © 2009 International Astronomical Union
We are performing a uniform and unbiased, ~7x7 degrees imaging survey of the Large Magellanic Cloud ...
We are performing a uniform and unbiased imaging survey of the Large Magellanic Cloud (LMC; ~7° × 7°...
We have used the Infrared Spectrograph (IRS) on the Spitzer Space Telescope to observe stars in the ...
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust...
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust...
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust...
International audienceThe Small Magellanic Cloud (SMC) provides a unique laboratory for the study of...
The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spit...
The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spit...
The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to the SAGE-LMC photometric survey...
The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to the SAGE-LMC photometric survey...
International audienceWe investigate the infrared (IR) properties of cool, evolved stars in the Smal...
We have imaged the entire Small Magellanic Cloud (SMC), one of the two nearest star-forming dwarf ga...
http://arxiv.org/abs/1004.1142The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to t...
We have imaged the entire Small Magellanic Cloud (SMC), one of the two nearest star-forming dwarf ga...
We are performing a uniform and unbiased, ~7x7 degrees imaging survey of the Large Magellanic Cloud ...
We are performing a uniform and unbiased imaging survey of the Large Magellanic Cloud (LMC; ~7° × 7°...
We have used the Infrared Spectrograph (IRS) on the Spitzer Space Telescope to observe stars in the ...
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust...
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust...
The Small Magellanic Cloud (SMC) provides a unique laboratory for the study of the lifecycle of dust...
International audienceThe Small Magellanic Cloud (SMC) provides a unique laboratory for the study of...
The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spit...
The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spit...
The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to the SAGE-LMC photometric survey...
The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to the SAGE-LMC photometric survey...
International audienceWe investigate the infrared (IR) properties of cool, evolved stars in the Smal...
We have imaged the entire Small Magellanic Cloud (SMC), one of the two nearest star-forming dwarf ga...
http://arxiv.org/abs/1004.1142The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to t...
We have imaged the entire Small Magellanic Cloud (SMC), one of the two nearest star-forming dwarf ga...
We are performing a uniform and unbiased, ~7x7 degrees imaging survey of the Large Magellanic Cloud ...
We are performing a uniform and unbiased imaging survey of the Large Magellanic Cloud (LMC; ~7° × 7°...
We have used the Infrared Spectrograph (IRS) on the Spitzer Space Telescope to observe stars in the ...