Andrea Miglio
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
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
Dr Fiorenzo Vincenzo F.Vincenzo@hull.ac.uk
Lecturer in Astrophysics
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 |
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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/.
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