Mapping the Galactic Halo with SDSS, LINEAR and PTF RR Lyrae Stars

Details Mapping the Galactic Halo with SDSS, LINEAR and PTF RR Lyrae Stars Mapping the Galactic Halo with SDSS, LINEAR and PTF RR Lyrae Stars

2011-05-20

arxiv.org/abs/1105.4146v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

To appear in the Carnegie Observatories Astrophysics Series, Volume 5

Scientific paper

We present an analysis of Galactic halo structure and substructure traced by ~500 RR Lyrae stars in the SDSS stripe 82 region. The main result of this study is a 2D map of the Galactic halo that reaches distances of 100 kpc and traces previously known and new halo substructures, such as the Sagittarius and Pisces tidal streams. We also present strong direct evidence, based on both RR Lyrae and main sequence stars, that the halo stellar number density profile significantly steepens beyond 30 kpc from the Galactic center. Using a novel photometric metallicity method that simultaneously combines data for RR Lyrae and main sequence stars, we show that the median metallicity of the Sagittarius trailing stream in the SDSS stripe 82 region is [Fe/H]}=-1.2 +- 0.1 dex. In addition to these results, we will present ongoing work on a 3D map of the Galactic halo constructed using a sample of ~4000 RR Lyrae stars that covers 8500 deg^2 of northern sky and probes up to 30 kpc from the Sun.

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