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The Three-Dimensional Structure of Cassiopeia A
Tracey DeLaney, Lawrence Rudnick, M. D. Stage +9
We used the Spitzer Space Telescope's Infrared Spectrograph to map nearly the entire extent of Cassiopeia A between 5-40 micron. Using infrared and Chandra X-ray Doppler velocity m…
Statistical study of dust properties in LMC molecular clouds
D. Paradis, W. T. Reach, J. P. Bernard +6
The objective of this paper is to construct a catalog providing the dust properties and the star formation efficiency (SFE) of the molecular clouds in the Large Magellanic Cloud (L…
Dust emission and star formation in Stephan's Quintet
G. Natale, R. J. Tuffs, C. K. Xu +11
We analyse a comprehensive set of MIR/FIR observations of Stephan's Quintet (SQ), taken with the Spitzer Space Observatory. Our study reveals the presence of a luminous (L_{IR}\app…
The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification I
Paul M. Woods, J. M. Oliveira, F. Kemper +55
We present the classification of 197 point sources observed with the Infrared Spectrograph in the SAGE-Spec Legacy program on the Spitzer Space Telescope. We introduce a decision-t…
Sub-millimeter to centimeter excess emission from the Magellanic Clouds. I. Global spectral energy distribution
F. P. Israel, W. F. Wall, D. Raban +5
In order to reconstruct the global SEDs of the Magellanic Clouds over eight decades in spectral range, we combined literature flux densities representing the entire LMC and SMC res…
The Three-Dimensional Structure of Interior Ejecta in Cassiopeia A at High Spectral Resolution
Karl Isensee, Lawrence Rudnick, Tracey DeLaney +5
We used the Spitzer Space Telescope's Infrared Spectrograph to create a high resolution spectral map of the central region of the Cassiopeia A supernova remnant, allowing us to mak…