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20242026
most citedNot all nitrogen-rich field stars originate from globular clusters

1 citations · 1 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20261 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.HE2026

AGN in Gaia Alerts: from flares to Changing Look Quasars

M. Dennefeld, T. Pursimo, C. Carvalho +11

The Gaia Alerts system is providing alerts on a variety of objects displaying a significant photometric change detected by the Gaia satellite from one passage to the next one over…

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.SR2025

DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations

A. Mazzi, J. S. Thomsen, A. Miglio +5

Asteroseismology gives us the opportunity to better characterize binaries and their products, and shed light on their role in Galactic populations. We estimate occurrence rates, ma…

astro-ph.SR2025

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.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…