Extended main-sequence turnoff and red clump in intermediate-age star clusters: A study of NGC 419
Journal
Date Issued
2023
Author(s)
Dresbach, F.
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•
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Ferraro, Francesco R.
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•
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Raso, S.
Abstract
With the goal of untangling the origin of extended main-sequence turnoffs
(eMSTOs) and extended red clumps (eRCs) in star clusters, in this work we
present the study of the intermediate-age cluster NGC 419, situated along the
Bridge of the Small Magellanic Cloud. To this aim, we analyzed multi-epoch,
high angular resolution observations acquired with the Hubble Space Telescope
for this dynamically young cluster, which enabled the determination of precise
proper motions and therefore the assessment of the cluster membership for each
individual star in the field of view. With this unprecedented information at
hand, we first studied the radial distribution of kinematically selected member
stars in different eMSTO subregions. The absence of segregation supports the
rotation scenario as the cause for the turnoff color extension and disfavors
the presence of a prolonged period of star formation in the cluster. A similar
analysis on the eRC of NGC 419 confirms the absence of segregation, providing
further evidence against an age spread, which is at odds with previous
investigations. Even so, the currently available evolutionary models including
stellar rotation fail at reproducing the two photometric features
simultaneously. We argue that either shortcomings in these models or a
different origin for the red clump feature, such as a nonstandard differential
mass loss along the red giant branch phase, are the only way to reconcile our
observational findings with theoretical expectations.
Volume
679
Start page
A102
Issn Identifier
0004-6361
Rights
open.access
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