Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-11T05:44:51.174Z Has data issue: false hasContentIssue false

Oxygen-rich Long Period Variables in the X-Shooter Spectral Library

Published online by Cambridge University Press:  30 December 2019

Ariane Lançon
Affiliation:
Université de Strasbourg, CNRS, UMR7550, Observatoire astronomique de Strasbourg, 67000 Strasbourg, France email: ariane.lancon@astro.unistra.fr
Anas Gonneau
Affiliation:
Institute of Astronomy, University of Cambridge, United Kingdom
Scott C. Trager
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, The Netherlands
Philippe Prugniel
Affiliation:
Centre de Recherche Astrophysique de Lyon (UMR 5574), Université de Lyon, France
Anke Arentsen
Affiliation:
Leibniz-Institut für Astrophysik Potsdam, Germany
Yanping Chen
Affiliation:
New York University in Abu Dhabi, United Arab Emirates
Matthijs Dries
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, The Netherlands
Cécile Loup
Affiliation:
Université de Strasbourg, CNRS, UMR7550, Observatoire astronomique de Strasbourg, 67000 Strasbourg, France email: ariane.lancon@astro.unistra.fr
Mariya Lyubenova
Affiliation:
European Southern Observatory, Garching, Germany
Reynier Peletier
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, The Netherlands
Laure Telliez
Affiliation:
Université de Strasbourg, CNRS, UMR7550, Observatoire astronomique de Strasbourg, 67000 Strasbourg, France email: ariane.lancon@astro.unistra.fr
Alexandre Vazdekis
Affiliation:
Instituto de Astrofisica de Canarias, Santa Cruz de Tenerife, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Bladh, S., Höfner, S., Aringer, B., & Eriksson, K. 2015, A&A, 575, A105 Google Scholar
Chen, Y.-P., Trager, S.C., Peletier, R.F. et al. 2014, A&A, 565, A117 Google Scholar
Gonneau, A., Lançon, A., Trager, S.C., Aringer, B., et al. 2016, A&A, 589, A36 Google Scholar
Gonneau, A., Lançon, A., Trager, S.C., Aringer, B., et al. 2017, A&A, 601, A141 Google Scholar
Husser, T.-O., Wende-von Berg, S., Dreizler, S. et al. 2013, A&A, 553, A6 Google Scholar
Lançon, A., & Wood, P. 2000, A&AS, 146, 217 Google Scholar
Lançon, A., & Mouhcine, M. 2002, A&A, 393, 167 Google Scholar
Powalka, M., Lançon, A., Puzia, T.H., et al. 2016, ApJS, 227, 12 CrossRefGoogle Scholar
Wing, R.F. 1974, HiA, 3, 285 Google Scholar