Samenvatting
The X-Shooter Spectral Library (XSL) contains more than 800 spectra of stars across the color-magnitude diagram, that extend from near-UV to near-IR wavelengths (320-2450 nm). We summarize properties of the spectra of O-rich Long Period Variables in the XSL, such as phase- related features, and we confront the data with synthetic spectra based on static and dynamical stellar atmosphere models. We discuss successes and remaining discrepancies, keeping in mind the applications to population synthesis modeling that XSL is designed for.
Originele taal-2 | English |
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Titel | Proceedings of the International Astronomical Union Volume 14 symposium s343: why galaxies care about agb stars: a continuing . |
Redacteuren | F. Kerschbaum, M. Groenewegen, H. Oloffson |
Uitgeverij | International Astronomical Union |
Pagina's | 309-313 |
Aantal pagina's | 5 |
Volume | 14 |
Uitgave | Symposium 343 |
DOI's | |
Status | Published - 1-dec.-2019 |
Evenement | IAUS 343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time - Vienna, Austria Duur: 20-aug.-2018 → 23-aug.-2018 |
Conference
Conference | IAUS 343: Why Galaxies Care About AGB Stars |
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Land/Regio | Austria |
Stad | Vienna |
Periode | 20/08/2018 → 23/08/2018 |