The Millennium Galaxy Catalogue: Star counts and the Structure of the Galactic Stellar Halo

Details The Millennium Galaxy Catalogue: Star counts and the Structure of the Galactic Stellar Halo The Millennium Galaxy Catalogue: Star counts and the Structure of the Galactic Stellar Halo

2003-08-12

arxiv.org/abs/astro-ph/0308200v1

Mon.Not.Roy.Astron.Soc.347:1043,2004

Astronomy and Astrophysics

Astrophysics

Accepted for publication in MNRAS (figs 16 and 17 degraded here)

Scientific paper

10.1111/j.1365-2966.2004.07065.x

We derive a star catalogue generated from the images taken as part of the 37.5 sq. deg Millennium Galaxy Catalogue. These data, alone and together with colours gained from the Sloan Digital Sky Survey Early Data Release, allow the analysis of faint star counts (B(MGC) < 20) at high Galactic latitude (41 < b < 63), as a function of Galactic longitude (239 < l < 353). We focus here on the inner stellar halo, providing robust limits on the amplitude of substructure and on the large-scale flattening. In line with previous results, the thick disk, an old, intermediate-metallicity population, is clearly seen in the colour-magnitude diagram. We find that the Galactic stellar halo within ~10 kpc (the bulk of the stellar mass) is significantly flattened, with an axial ratio of (c/a) =0.56 +/- 0.01, again consistent with previous results. Our analysis using counts-in-cells, angular correlation functions and the Lee 2D statistic, confirms tidal debris from the Sagittarius dwarf but finds little evidence for other substructure in the inner halo, at heliocentric distances of < 5 kpc. This new quantification of the smoothness in coordinate space limits the contribution of recent accretion/disruption to the build-up of the bulk of the stellar halo.

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