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: | , , , , , , , , , , , |
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| Dokumenttyp: | Article (Journal) Konferenzschrift |
| Sprache: | Englisch |
| Veröffentlicht: |
02 August 2018
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| 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 
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| 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 |
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| 520 | |a 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. | ||
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| 700 | 1 | |a Mor, R. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Bono, G. |e VerfasserIn |4 aut | |
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| 700 | 1 | |a Robin, A. C. |e VerfasserIn |4 aut | |
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