Haydn

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; Fiorenzo Vincenzo

doi:10.1007/s10686-021-09711-1

Haydn

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 MagrinGeorges Meynet, Eric Michel, Josefina Montalbán, Valerio Nascimbeni, Arlette Noels, Giampaolo Piotto, Roberto Ragazzoni, Igor Soszyński, Eline Tolstoy, Silvia Toonen, Amaury Triaud, Fiorenzo Vincenzo

^*Corresponding author voor dit werk

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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.

Originele taal-2	English
Pagina's (van-tot)	963-1001
Aantal pagina's	39
Tijdschrift	Experimental Astronomy
Volume	51
DOI's	https://doi.org/10.1007/s10686-021-09711-1
Status	Published - 1-jun.-2021

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10.1007/s10686-021-09711-1Licentie: CC BY

HAYDN High-precision AsteroseismologY of DeNse stellar fieldsFinal publisher's version, 1,34 MBLicentie: CC BY

https://ui.adsabs.harvard.edu/abs/2021ExA....51..963M

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Miglio, A., Girardi, L., Grundahl, F., Mosser, B., Bastian, N., Bragaglia, A., Brogaard, K., Buldgen, G., Chantereau, W., Chaplin, W., Chiappini, C., Dupret, M.-A., Eggenberger, P., Gieles, M., Izzard, R., Kawata, D., Karoff, C., Lagarde, N., Mackereth, T., ... Vincenzo, F. (2021). Haydn. Experimental Astronomy, 51, 963-1001. https://doi.org/10.1007/s10686-021-09711-1

@article{ea6df7e089a54498b5deea3929d3c1f9,

title = "Haydn",

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.",

keywords = "Stars: low-mass, Globular clusters, Galaxy: bulge, Galaxies: dwarf, Asteroseismology, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies",

author = "Andrea Miglio and L{\'e}o Girardi and Frank Grundahl and Benoit Mosser and Nate Bastian and Angela Bragaglia and Karsten Brogaard and Ga{\"e}l Buldgen and William Chantereau and William Chaplin and Cristina Chiappini and Marc-Antoine Dupret and Patrick Eggenberger and Mark Gieles and Robert Izzard and Daisuke Kawata and Christoffer Karoff and Nad{\`e}ge Lagarde and Ted Mackereth and Demetrio Magrin and Georges Meynet and Eric Michel and Josefina Montalb{\'a}n and Valerio Nascimbeni and Arlette Noels and Giampaolo Piotto and Roberto Ragazzoni and Igor Soszy{\'n}ski and Eline Tolstoy and Silvia Toonen and Amaury Triaud and Fiorenzo Vincenzo",

year = "2021",

month = jun,

day = "1",

doi = "10.1007/s10686-021-09711-1",

language = "English",

volume = "51",

pages = "963--1001",

journal = "Experimental Astronomy",

issn = "0922-6435",

publisher = "Springer",

}

Miglio, A, Girardi, L, Grundahl, F, Mosser, B, Bastian, N, Bragaglia, A, Brogaard, K, Buldgen, G, Chantereau, W, Chaplin, W, Chiappini, C, Dupret, M-A, Eggenberger, P, Gieles, M, Izzard, R, Kawata, D, Karoff, C, Lagarde, N, Mackereth, T, Magrin, D, Meynet, G, Michel, E, Montalbán, J, Nascimbeni, V, Noels, A, Piotto, G, Ragazzoni, R, Soszyński, I, Tolstoy, E, Toonen, S, Triaud, A & Vincenzo, F 2021, 'Haydn', Experimental Astronomy, vol. 51, blz. 963-1001. https://doi.org/10.1007/s10686-021-09711-1

TY - JOUR

T1 - Haydn

AU - Miglio, Andrea

AU - Girardi, Léo

AU - Grundahl, Frank

AU - Mosser, Benoit

AU - Bastian, Nate

AU - Bragaglia, Angela

AU - Brogaard, Karsten

AU - Buldgen, Gaël

AU - Chantereau, William

AU - Chaplin, William

AU - Chiappini, Cristina

AU - Dupret, Marc-Antoine

AU - Eggenberger, Patrick

AU - Gieles, Mark

AU - Izzard, Robert

AU - Kawata, Daisuke

AU - Karoff, Christoffer

AU - Lagarde, Nadège

AU - Mackereth, Ted

AU - Magrin, Demetrio

AU - Meynet, Georges

AU - Michel, Eric

AU - Montalbán, Josefina

AU - Nascimbeni, Valerio

AU - Noels, Arlette

AU - Piotto, Giampaolo

AU - Ragazzoni, Roberto

AU - Soszyński, Igor

AU - Tolstoy, Eline

AU - Toonen, Silvia

AU - Triaud, Amaury

AU - Vincenzo, Fiorenzo

PY - 2021/6/1

Y1 - 2021/6/1

N2 - 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.

AB - 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.

KW - Stars: low-mass

KW - Globular clusters

KW - Galaxy: bulge

KW - Galaxies: dwarf

KW - Asteroseismology

KW - Astrophysics - Solar and Stellar Astrophysics

KW - Astrophysics - Astrophysics of Galaxies

U2 - 10.1007/s10686-021-09711-1

DO - 10.1007/s10686-021-09711-1

M3 - Article

SN - 0922-6435

VL - 51

SP - 963

EP - 1001

JO - Experimental Astronomy

JF - Experimental Astronomy

ER -

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