Skip to main content

Research Repository

Advanced Search

HAYDN: High-precision AsteroseismologY of DeNse stellar fields

Miglio, Andrea; Girardi, Léo; Grundahl, Frank; Mosser, Benoit; Bastian, Nate; Bragaglia, Angela; Brogaard, Karsten; Buldgen, Gaël; Chantereau, William; Chaplin, William; Chiappini, Cristina; Dupret, Marc-Antoine; 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

Authors

Andrea Miglio

Léo Girardi

Frank Grundahl

Benoit Mosser

Nate Bastian

Angela Bragaglia

Karsten Brogaard

Gaël Buldgen

William Chantereau

William Chaplin

Cristina Chiappini

Marc-Antoine Dupret

Patrick Eggenberger

Mark Gieles

Robert Izzard

Daisuke Kawata

Christoffer Karoff

Nadège Lagarde

Ted Mackereth

Demetrio Magrin

Georges Meynet

Eric Michel

Josefina Montalbán

Valerio Nascimbeni

Arlette Noels

Giampaolo Piotto

Roberto Ragazzoni

Igor Soszyński

Eline Tolstoy

Silvia Toonen

Amaury Triaud



Abstract

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.

Citation

Miglio, A., Girardi, L., Grundahl, F., Mosser, B., Bastian, N., Bragaglia, A., …Vincenzo, F. (2021). HAYDN: High-precision AsteroseismologY of DeNse stellar fields. Experimental astronomy, 51(3), 963-1001. https://doi.org/10.1007/s10686-021-09711-1

Journal Article Type Article
Acceptance Date Feb 9, 2021
Online Publication Date Mar 26, 2021
Publication Date 2021-06
Deposit Date Mar 12, 2022
Publicly Available Date Mar 16, 2022
Journal Experimental Astronomy
Print ISSN 0922-6435
Electronic ISSN 1572-9508
Publisher Springer Verlag
Peer Reviewed Peer Reviewed
Volume 51
Issue 3
Pages 963-1001
DOI https://doi.org/10.1007/s10686-021-09711-1
Keywords Stars: low-mass; Globular clusters; Galaxy: bulge; Galaxies: dwarf; Asteroseismology
Public URL https://hull-repository.worktribe.com/output/3948282
Additional Information Received: 29 July 2020; Accepted: 9 February 2021; First Online: 26 March 2021

Files

Published article (1.4 Mb)
PDF

Copyright Statement
© The Author(s) 2021.
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4. 0/.





You might also like



Downloadable Citations