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Andromeda IX: Properties of the Smallest M 31 Dwarf Satellite Galaxy

D. Harbeck·J. Gallagher·E. K. Grebel·A. Koch·D. Zucker
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Abstract

We present WIYN observations of the recently discovered And IX dwarf spheroidal (dSph) satellite galaxy of M 31. Our data, obtained at a natural seeing of 0.5'' and just reaching the horizontal branch level, confirm And IX as a dSph galaxy with a distance similar to M 31. A survey for carbon stars shows no evidence for an intermediate-age (1--10 Gyr) stellar population in And IX. From the red giant branch we estimate a metallicity of roughly -2 dex. Combined with the tip of the red giant branch luminosity, this results in a distance of 735 kpc, placing And IX approximately 45 kpc from M 31. This faint dSph follows the relations between luminosity and metallicity, and luminosity and surface brightness defined by other Local Group dSph galaxies. The core and tidal radii are found to be 1.35' and 5.9', respectively. We conclude that And IX -- despite its low luminosity -- might be an ordinary Local Group dSph and discuss implications for its formation from a once more massive, but stripped progenitor or from an intrinsically low-mass seed.

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D. Harbeck, J. Gallagher, E. K. Grebel, A. Koch, D. Zucker. 2005-01-20. Andromeda IX: Properties of the Smallest M 31 Dwarf Satellite Galaxy. https://doi.org/10.1086/428650

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