Project Details
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Shaping Our Galaxy Now: The Low-Latitude Stellar Stream around the Milky Way

Subject Area Astrophysics and Astronomy
Term from 2005 to 2010
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 5448769
 
Final Report Year 2012

Final Report Abstract

The project set out to develop and implement approaches to find, map and interpret stellar substructure in the outskirts of our Milky Way, which serve as a signpost and a diagnostic of hierarchical galaxy formation in our immediate cosmic neighborhood. In particular, the project has focussed on a comprehensive empirical picture of the Low Latitude stellar stream around the MW and its possible progenitor, the Canis Major stellar overdensity (CMa). For its data, the project has drawn on SDSS/SEGUE imaging data, increasingly supplemented by follow-up imaging in the second part of the SPP. On that basis we were able to develop optimal techniques to find stellar streams in the Milky Way, to characterize and model them; and the project has produced the state of the art map of the ‘Monoceros stream’, showing that it actually encircles much of the Galaxy, that it cannot be modeled as a simple warp or flare, and that it exhibits a distinct stellar metallicity structure. Overall, these results established a picture of a complex outer MW disk, which is indeed undergoing significant tidal interaction.

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