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| EPoS Contribution |
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Star formation and disk evolution in the Coronet cluster
Aurora Sicilia-Aguilar Max-Planck-Institut für Astronomie, Heidelberg, Germany | |
| The Coronet cluster is a young low-mass star forming region located at 170 pc distance within the Corona Australis cloud. It contains objects in all stages of evolution, from Class 0/I protostars to Class III pre-main sequence stars without disks, being an ideal target to study the formation and evolution of low-mass objects. I will present the results of our multiwavelength study, which includes optical spectroscopy, Spitzer (IRAC, MIPS, and IRS) data, APEX/LABOCA submillimeter data, and Herschel/PACS observations. | |
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| Caption: APEX/LABOCA 870$\mu$m contours over a Spitzer three color image (4.5, 8.0, and 24 micron) of the Coronet Cluster. | |
| Collaborators: Th. Henning, MPIA, Germany J. Bouwman, MPIA, Germany O. Krause, MPIA, Germany |
Suggested Session:
Early Phases of Disks, Molecular Clouds, Herschel |