Blue straggler stars in dwarf spheroidal galaxies II: Sculptor and Fornax
M. Mapelli, E. Ripamonti, G. Battaglia, E. Tolstoy, M. J. Irwin, B., Moore, S. Sigurdsson

TL;DR
This study investigates blue straggler star candidates in the dwarf spheroidal galaxies Sculptor and Fornax, analyzing their distributions to determine their nature and implications for galaxy star formation histories.
Contribution
It provides a comparative analysis of BSS candidates in Sculptor and Fornax, distinguishing between genuine BSSs and young stars based on spatial distributions and theoretical models.
Findings
In Sculptor, BSS candidates match the distribution of RHB stars, supporting a binary mass transfer origin.
In Fornax, BSS candidates are more centrally concentrated, indicating they are likely young stars.
Sculptor shows no evidence of recent star formation, unlike Fornax.
Abstract
The existence of blue straggler stars (BSSs) in dwarf spheroidal galaxies (dSphs) is still an open question. In fact, many BSS candidates have been observed in the Local Group dSphs, but it is unclear whether they are real BSSs or young stars. Shedding light on the nature of these BSS candidates is crucial, in order to understand the star formation history of dSphs. In this paper, we consider BSS candidates in Sculptor and Fornax. In Fornax there are strong hints that the BSS population is contaminated by young stars, whereas in Sculptor there is no clear evidence of recent star formation. We derive the radial and luminosity distribution of BSS candidates from wide field imaging data extending beyond the nominal tidal radius of these galaxies. The observations are compared with the radial distribution of BSSs expected from dynamical simulations. In Sculptor the radial distribution of…
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