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20212026
most citedAsteroseismology of the multiple stellar populations in the Globular Cluster M4

33 citations · 113 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026★ 1 cited

Not all nitrogen-rich field stars originate from globular clusters

Ellen I. Leitinger, Andrea Miglio, Josefina Montalbán +7

Globular clusters (GCs) are important tracers of the early Galactic assembly process, with part of their stars showing distinct chemical abundance patterns. When such stars are fou…

astro-ph.SR2025★ 7 cited

Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary

J. S. Thomsen, A. Miglio, K. Brogaard +26

The study of resonant oscillation modes in low-mass red giant branch stars enables their ages to be inferred with exceptional (10%) precision, unlocking the possibility to re…

astro-ph.GA2024

Tracing back a second-generation star stripped from Terzan 5 by the Galactic bar

Stefano O. Souza, Marica Valentini, Cristina Chiappini +6

The Galactic bulge hosts the Milky Way's oldest stars, possibly coming from disrupted globular clusters (GCs) or the bulge's primordial building blocks, making these stars witnesse…

astro-ph.SR2024★ 7 cited

Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product

Massimiliano Matteuzzi, David Hendriks, Robert G. Izzard +5

Precise masses of red-giant stars enable a robust inference of their ages, but there are cases where these age estimates are highly precise yet very inaccurate. Examples are core-h…

astro-ph.GA2024★ 33 cited

Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS

Samir Nepal, Cristina Chiappini, Anna B. A. Queiroz +5

JWST has recently detected numerous disc galaxies at high-redshifts and there have been observations of cold disc galaxies at z > 4 with ALMA. In the Milky Way, recent studies find…

astro-ph.GA2023

K2 results for "young" -rich stars in the Galaxy

V. Grisoni, C. Chiappini, A. Miglio +11

The origin of apparently young -rich stars in the Galaxy is still a matter of debate in Galactic archaeology, whether they are genuinely young or might be products of binary evo…

astro-ph.GA2023★ 2 cited

Beyond Gaia DR3: Tracing the [/M]-[M/H] bimodality from the inner to the outer Milky Way disc with Gaia-RVS and convolutional neural networks

G. Guiglion, S. Nepal, C. Chiappini +17

In June 2022, Gaia DR3 has provided the astronomy community with about one million spectra from the Radial Velocity Spectrometer (RVS) covering the CaII triplet region. However, on…

astro-ph.SR2023★ 16 cited

Red Horizontal Branch stars: an asteroseismic perspective

Massimiliano Matteuzzi, Josefina Montalbán, Andrea Miglio +7

Robust age estimates of red giant stars are now possible thanks to the precise inference of their mass based on asteroseismic constraints. However, there are cases where such age e…

astro-ph.SR2022★ 33 cited

Asteroseismology of the multiple stellar populations in the Globular Cluster M4

M. Tailo, E. Corsaro, A. Miglio +6

We present a new asteroseismic analysis of the stars in the Globular Cluster (GC) M4 based on the data collected by the K2 mission. We report the detection of solar-like oscillatio…

astro-ph.SR2021★ 14 cited

Asteroseismology of Cephei stars: The stellar inferences tested in hare and hound exercises

Sébastien Salmon, Patrick Eggenberger, Josefina Montalbán +5

The Cephei pulsators are massive main-sequence stars, presenting low radial-order modes. These modes probe in particular the chemical gradient at the edge of the convective cor…