activity
20242026
collaborators

5 papers

astro-ph.SR2026

Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS

Emma Willett, Andrea Miglio, Saniya Khan +9

The availability of asteroseismic constraints for tens of thousands of red giant (RG) stars has opened the door to robust age estimates, enabling time-resolved studies of different…

astro-ph.GA2026

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

Attempting an accurate age estimate of the open cluster NGC 6633 using CoRoT and Gaia

K. Brogaard, A. Miglio, T. Arentoft +5

Asteroseismology of solar-like oscillations in giant stars allow the derivation of their masses and radii. For members of open clusters, this provides an age of the cluster that sh…

astro-ph.GA2025

Tracing the Milky Way: Calibrating chemical ages with high-precision Kepler data

G. Casali, J. Montalbà n, A. Miglio +10

Chemical clocks offer a powerful tool for estimating stellar ages from spectroscopic surveys. We present a new detailed spectroscopic analysis of 68 Kepler red giant stars to provi…

astro-ph.SR2024

Connecting integrated RGB mass loss from asteroseismology and globular clusters

K. Brogaard, A. Miglio, W. E. van Rossem +2

Context. Asteroseismic investigations of solar-like oscillations in giant stars enable the derivation of their masses and radii. For mono-age mono-metallicity populations of stars…