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Cepheids as Swiss army knives for Milky Way archaeology

Cepheids are excellent stellar tracers: they are bright enough to be observed even at large distances; their distances can be accurately determined via period-luminosity relations; their spectra contain numerous lines that enable us to derive abundances for many α, iron-peak or neutron-capture eleme...

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Hauptverfasser: Lemasle, Bertrand (VerfasserIn) , Kovtyukh, Valery (VerfasserIn) , Silva, R. da (VerfasserIn) , Mor, R. (VerfasserIn) , Bono, G. (VerfasserIn) , Figueras, F. (VerfasserIn) , François, P. (VerfasserIn) , Inno, L. (VerfasserIn) , Magurno, D. (VerfasserIn) , Matsunaga, N. (VerfasserIn) , McWilliam, A. (VerfasserIn) , Robin, A. C. (VerfasserIn)
Dokumenttyp: Article (Journal) Konferenzschrift
Sprache:Englisch
Veröffentlicht: 02 August 2018
In: Proceedings of the International Astronomical Union
Year: 2017, Jahrgang: 13, Heft: S334, Pages: 329-330
ISSN:1743-9221
DOI:10.1017/S1743921317007451
Online-Zugang:Verlag, Volltext: https://doi.org/10.1017/S1743921317007451
Verlag, Volltext: https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/cepheids-as-swiss-army-knives-for-milky-way-archaeology/FC0F39FC66B1FBB18642A5572CA363EF
Volltext
Verfasserangaben:B. Lemasle, V. Kovtyukh, R. da Silva, R. Mor, G. Bono, F. Figueras, P. François, L. Inno, D. Magurno, N. Matsunaga, A. McWilliam and A.C. Robin
Beschreibung
Zusammenfassung:Cepheids are excellent stellar tracers: they are bright enough to be observed even at large distances; their distances can be accurately determined via period-luminosity relations; their spectra contain numerous lines that enable us to derive abundances for many α, iron-peak or neutron-capture elements. Classical Cepheids are yellow supergiants that trace the young populations (⩽ 300 Myr); Type II Cepheids are post Horizontal Branch, low-mass, Population II stars (⩾ 10 Gyr). Both can be used for many purposes in Milky Way archaeology.
Beschreibung:Gesehen am 03.09.2019
Beschreibung:Online Resource
ISSN:1743-9221
DOI:10.1017/S1743921317007451

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