HAYDN

In the last decade, the Kepler and CoRoT space-photometry missions have demonstrated the potential of asteroseismology as a novel, versatile and powerful tool to perform exquisite tests of stellar physics, and to enable precise and accurate characterisations of stellar properties, with impact on bot...

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Veröffentlicht in:Experimental astronomy 2021-06, Vol.51 (3), p.963-1001
Hauptverfasser: Miglio, Andrea, Girardi Léo, Grundahl, Frank, Mosser Benoit, Bastian, Nate, Bragaglia Angela, Brogaard Karsten, Buldgen Gaël, Chantereau, William, Chaplin, William, Chiappini, Cristina, Marc-Antoine, Dupret, Eggenberger, Patrick, Gieles, Mark, Izzard, Robert, Kawata Daisuke, Karoff Christoffer, Lagarde Nadège, Mackereth, Ted, Magrin Demetrio, Meynet Georges, Michel, Eric, Montalbán Josefina, Nascimbeni Valerio, Noels Arlette, Piotto Giampaolo, Ragazzoni, Roberto, Soszyński Igor, Tolstoy Eline, Toonen, Silvia, Triaud Amaury, Vincenzo Fiorenzo
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container_title Experimental astronomy
container_volume 51
creator Miglio, Andrea
Girardi Léo
Grundahl, Frank
Mosser Benoit
Bastian, Nate
Bragaglia Angela
Brogaard Karsten
Buldgen Gaël
Chantereau, William
Chaplin, William
Chiappini, Cristina
Marc-Antoine, Dupret
Eggenberger, Patrick
Gieles, Mark
Izzard, Robert
Kawata Daisuke
Karoff Christoffer
Lagarde Nadège
Mackereth, Ted
Magrin Demetrio
Meynet Georges
Michel, Eric
Montalbán Josefina
Nascimbeni Valerio
Noels Arlette
Piotto Giampaolo
Ragazzoni, Roberto
Soszyński Igor
Tolstoy Eline
Toonen, Silvia
Triaud Amaury
Vincenzo Fiorenzo
description In the last decade, the Kepler and CoRoT space-photometry missions have demonstrated the potential of asteroseismology as a novel, versatile and powerful tool to perform exquisite tests of stellar physics, and to enable precise and accurate characterisations of stellar properties, with impact on both exoplanetary and Galactic astrophysics. Based on our improved understanding of the strengths and limitations of such a tool, we argue for a new small/medium space mission dedicated to gathering high-precision, high-cadence, long photometric series in dense stellar fields. Such a mission will lead to breakthroughs in stellar astrophysics, especially in the metal poor regime, will elucidate the evolution and formation of open and globular clusters, and aid our understanding of the assembly history and chemodynamics of the Milky Way’s bulge and a few nearby dwarf galaxies.
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subjects Astrophysics
Dwarf galaxies
Extrasolar planets
Globular clusters
Photometry
Sciences of the Universe
Space missions
Stellar evolution
Stellar physics
Stellar seismology
title HAYDN
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