Photometric stellar parameters for asteroseismology and Galactic studies

Luca Casagrande

doi:10.1007/978-3-319-10993-0_7

Photometric stellar parameters for asteroseismology and Galactic studies

Luca Casagrande^*

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

2 Citations (Scopus)

Abstract

Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When coupling this information with classical determinations of stellar parameters, such as metallicities, effective temperatures and angular diameters, powerful new diagnostics for both stellar and Galactic studies can be obtained. I review how different photometric systems and filters carry important information on classical stellar parameters, the accuracy at which these parameters can be derived, and summarize some of the calibrations available in the literature for late-type stars. Recent efforts in combining classical and asteroseismic parameters are discussed, and the uniqueness of their intertwine is highlighted.

Original language	English
Title of host publication	Asteroseismology of Stellar Populations in the Milky Way
Editors	Andrea Miglio, Léo Girardi, Patrick Eggenberger, Josefina Montalban
Publisher	Kluwer Academic Publishers
Pages	61-71
Number of pages	11
ISBN (Print)	9783319109923
DOIs	https://doi.org/10.1007/978-3-319-10993-0_7
Publication status	Published - 2015
Event	Asteroseismology of Stellar Populations in the Milky Way Workshop, 2013 - Sexten, Italy Duration: 22 Jul 2013 → 26 Jul 2013

Publication series

Name	Astrophysics and Space Science Proceedings
Volume	39
ISSN (Print)	1570-6591
ISSN (Electronic)	1570-6605

Conference

Conference	Asteroseismology of Stellar Populations in the Milky Way Workshop, 2013
Country/Territory	Italy
City	Sexten
Period	22/07/13 → 26/07/13

Access to Document

10.1007/978-3-319-10993-0_7

Cite this

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title = "Photometric stellar parameters for asteroseismology and Galactic studies",

abstract = "Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When coupling this information with classical determinations of stellar parameters, such as metallicities, effective temperatures and angular diameters, powerful new diagnostics for both stellar and Galactic studies can be obtained. I review how different photometric systems and filters carry important information on classical stellar parameters, the accuracy at which these parameters can be derived, and summarize some of the calibrations available in the literature for late-type stars. Recent efforts in combining classical and asteroseismic parameters are discussed, and the uniqueness of their intertwine is highlighted.",

author = "Luca Casagrande",

note = "Publisher Copyright: {\textcopyright} Springer International Publishing Switzerland 2015.; Asteroseismology of Stellar Populations in the Milky Way Workshop, 2013 ; Conference date: 22-07-2013 Through 26-07-2013",

year = "2015",

doi = "10.1007/978-3-319-10993-0_7",

language = "English",

isbn = "9783319109923",

series = "Astrophysics and Space Science Proceedings",

publisher = "Kluwer Academic Publishers",

pages = "61--71",

editor = "Andrea Miglio and L{\'e}o Girardi and Patrick Eggenberger and Josefina Montalban",

booktitle = "Asteroseismology of Stellar Populations in the Milky Way",

}

Casagrande, L 2015, Photometric stellar parameters for asteroseismology and Galactic studies. in A Miglio, L Girardi, P Eggenberger & J Montalban (eds), Asteroseismology of Stellar Populations in the Milky Way. Astrophysics and Space Science Proceedings, vol. 39, Kluwer Academic Publishers, pp. 61-71, Asteroseismology of Stellar Populations in the Milky Way Workshop, 2013, Sexten, Italy, 22/07/13. https://doi.org/10.1007/978-3-319-10993-0_7

Photometric stellar parameters for asteroseismology and Galactic studies. / Casagrande, Luca.
Asteroseismology of Stellar Populations in the Milky Way. ed. / Andrea Miglio; Léo Girardi; Patrick Eggenberger; Josefina Montalban. Kluwer Academic Publishers, 2015. p. 61-71 (Astrophysics and Space Science Proceedings; Vol. 39).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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N2 - Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When coupling this information with classical determinations of stellar parameters, such as metallicities, effective temperatures and angular diameters, powerful new diagnostics for both stellar and Galactic studies can be obtained. I review how different photometric systems and filters carry important information on classical stellar parameters, the accuracy at which these parameters can be derived, and summarize some of the calibrations available in the literature for late-type stars. Recent efforts in combining classical and asteroseismic parameters are discussed, and the uniqueness of their intertwine is highlighted.

AB - Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When coupling this information with classical determinations of stellar parameters, such as metallicities, effective temperatures and angular diameters, powerful new diagnostics for both stellar and Galactic studies can be obtained. I review how different photometric systems and filters carry important information on classical stellar parameters, the accuracy at which these parameters can be derived, and summarize some of the calibrations available in the literature for late-type stars. Recent efforts in combining classical and asteroseismic parameters are discussed, and the uniqueness of their intertwine is highlighted.

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DO - 10.1007/978-3-319-10993-0_7

M3 - Conference contribution

SN - 9783319109923

T3 - Astrophysics and Space Science Proceedings

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BT - Asteroseismology of Stellar Populations in the Milky Way

A2 - Miglio, Andrea

A2 - Girardi, Léo

A2 - Eggenberger, Patrick

A2 - Montalban, Josefina

PB - Kluwer Academic Publishers

T2 - Asteroseismology of Stellar Populations in the Milky Way Workshop, 2013

Y2 - 22 July 2013 through 26 July 2013

ER -

Photometric stellar parameters for asteroseismology and Galactic studies

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