Measuring Substructure with SEGUE K Giants and BHB Stars

Details Measuring Substructure with SEGUE K Giants and BHB Stars Measuring Substructure with SEGUE K Giants and BHB Stars

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21922202m&link_type=abstract

American Astronomical Society, AAS Meeting #219, #222.02

Astronomy and Astrophysics

Astronomy

Scientific paper

New substructure measurements in the Milky Way halo will be presented, using the large samples of SEGUE K giants and BHB stars which stretch into the outer halo. We see interesting differences in substructure between inner and outer halo and between K stars and BHB stars, and report a new distant stream likely to be associated with the early disruption of the Sgr dwarf.

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