An extended stellar halo discovered in the Fornax dwarf spheroidal using Gaia EDR3
Yanbin Yang, Francois Hammer, Yongjun Jiao, Marcel Pawlowski

TL;DR
This study uses Gaia EDR3 data to identify an extended stellar halo in the Fornax dwarf galaxy, revealing a new component that extends far beyond its core and suggesting recent gas loss and a first infall scenario.
Contribution
The paper reports the discovery of an extended stellar halo in Fornax, significantly larger than previously known, using precise Gaia EDR3 data and star selection techniques.
Findings
Discovery of a stellar halo extending 5.4 kpc from Fornax center
The halo accounts for 10% of Fornax's stellar mass
No tidal features detected, implying a recent gas loss event
Abstract
We have studied the extent of the Red Giant Branch stellar population in the Fornax dwarf spheroidal galaxy using the spatially extended and homogeneous data set from Gaia EDR3. Our preselection of stars belonging to Fornax is based on their proper motions, parallaxes and color-magnitude diagram. The latter criteria provide a Fornax star sample, which we further restrict by color and magnitude to eliminate contaminations due to either Milky Way stars or QSOs. The precision of the data has been sufficient to reach extremely small contaminations (0.02 to 0.3%), allowing us to reach to a background level 12 magnitudes deeper than the central surface brightness of Fornax. We discover a break in the density profile, which reveals the presence of an additional component that extents 2.1 degree in radius, i.e. 5.4 kpc, and almost seven times the half-light radius of Fornax. The extended new…
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