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The Nuclear Structure of the Sagittarius Dwarf Spheroidal Galaxy

Lorenzo Monaco·Michele Bellazzini·Francesco R. Ferraro·Elena Pancino
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Abstract

We present a study of the central parts of the Sagittarius dwarf spheroidal galaxy (Sgr). We found a clear overdensity of Sgr's stars around M~54 (hereafter NS). NS is well represented by a King model and it has the characteristics of a typical dwarf elliptical nucleus. Whether this means that M~54 has spiraled into the potential well of NS or that M~54 is the real nucleus and NS has formed into its potential wells, remains an open question to be addressed.

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Lorenzo Monaco, Michele Bellazzini, Francesco R. Ferraro, Elena Pancino. 2003-09-02. The Nuclear Structure of the Sagittarius Dwarf Spheroidal Galaxy. https://arxiv.org/abs/astro-ph/0309044

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