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The Galaxys stellar populations are naturally classified into six `types, of which five have been observed. These are the thin disk (Pop I in the historical scheme), a discrete thick disk (Pop I.5), the metal-rich bulge, which was not named in the Baade sequence, the rare field halo (Pop II), a population currently being accreted into the very outer halo filed (Pop Sgr?)and a hard to discover initial enriching Pop III. Each of these forms a group with astonishly tight correlations between chemical element ratios and other parameters. It is very hard to understand how the observed properties of any one of these populations can be the sum of many discrete histories, except for the minor continuing outer halo accretion. All these stellar populations are embedded in dark-matter, and allow the properties of dark matter to be measured on small scales. Intriguing and unexpected consistencies in the properties of this dark matter are being revealed.
We use deep Hubble Space Telescope imaging in the outskirts of the nearby spiral M101 to study stellar populations in the galaxys outer disk and halo. Our ACS field lies 17.6 arcmin (36 kpc) from the center of M101 and targets the blue NE Plume of M1
By means of a semi-analytic model of galaxy formation, we show how the local observed relation between age and galactic stellar mass is affected by assuming a DM power spectrum with a small-scale cutoff. We compare results obtained by means of both a
We investigate the distribution of different classes of spectroscopically identified sources and theoretical models in the color-color diagrams (CCDs) combining the near-infrared (NIR) and mid-infrared (MIR) data to develop a method to classify Outer
We present HST photometry for three fields in the outer disk of the LMC extending approximately four magnitudes below the faintest main sequence turnoff. We cannot detect any strongly significant differences in the stellar populations of the three fi
The Dark Energy Camera has captured a large set of images as part of Science Verification (SV) for the Dark Energy Survey. The SV footprint covers a lar ge portion of the outer Large Magellanic Cloud (LMC), providing photometry 1.5 magnitudes fainter