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Andrea Miglio

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Professor

Università degli Studi di Bologna Dipartimento di Fisica e Astronomia

Italy

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About

Andrea Miglio is a Professor at the Università degli Studi di Bologna, Dipartimento di Fisica e Astronomia, Italy. His research focuses on stellar astronomy, particularly in the areas of stellar populations in clusters, asteroseismology, and the modeling of core-helium-burning stars. Recent publications include studies on rotational mixing in star clusters and the effects of convective-envelope overshooting in red giant branch stars.

Recent Grants

Grant: Close

Galactic archeology with high temporal resolution

Open Date: 2018-04-01

Close Date: 2023-09-30

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Collaborators (20)

Jo Bovy

University of Toronto

CANADA

Andrea Miglio

Research Interests

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About

Recent Grants

Articles (27)

The impact of rotational mixing in intermediate-age star clusters with extended main-sequence turn-offs and extended red clumps

Inferring the efficiency of convective-envelope overshooting in red giant branch stars

Parametric models of core-helium-burning stars: structural glitches near the core

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

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

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

Dissecting stellar populations with manifold learning

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

12C/13C of Kepler giant stars: The missing piece of the mixing puzzle

Insights from super-metal-rich stars: Is the Milky Way bar young?

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

Connecting integrated red giant branch mass loss from asteroseismology and globular clusters

Mixed-mode coupling in the red clump

Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS

Time evolution of Ce as traced by APOGEE using giant stars observed with the Kepler, TESS and K2 missions

The evolution of the Milky Way’s thin disc radial metallicity gradient with K2 asteroseismic ages

A variational encoder–decoder approach to precise spectroscopic age estimation for large Galactic surveys

Chasing the impact of the Gaia-Sausage-Enceladus merger on the formation of the Milky Way thick disc

Red horizontal branch stars: An asteroseismic perspective

Dissecting the <i>Gaia</i> HR diagram – II. The vertical structure of the star formation history across the solar cylinder

Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS

Seismic and spectroscopic analysis of nine bright red giants observed by Kepler

Asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia

Establishing the accuracy of asteroseismic mass and radius estimates of giant stars - II. Revised stellar masses and radii for KIC 8430105

Solar-like oscillations and ellipsoidal variations in TESS observations of the binary 12 Boötis

The distribution of [α/Fe] in the Milky Way disc

Asteroseismology of evolved stars to constrain the internal transport of angular momentum

Collaborators (20)

Jo Bovy

Alessio Mucciarelli

Stephanie Monty

J Ted Mackereth

Diego Bossini

Daisuke Kawata

Alexander J Lyttle

Karsten Brogaard

Samir Nepal

Benoit Mosser

Robert J J Grand

Sven Buder

Piero Dal Tio

Luca Casagrande

Jens Jessen-Hansen

Mikkel Nørup Lund

Matteo Dell'Omodarme

Valeria Grisoni

Amalie Stokholm

Richard I. Anderson

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