Hostname: page-component-77c89778f8-m8s7h Total loading time: 0 Render date: 2024-07-19T19:46:34.906Z Has data issue: false hasContentIssue false

TIGvival: High-resolution spectroscopic monitoring of LPV stars

Published online by Cambridge University Press:  30 December 2019

Uwe Wolter
Affiliation:
Hamburger Sternwarte, Universität Hamburg, Germany email: uwolter@hs.uni-hamburg.de
Dieter Engels
Affiliation:
Hamburger Sternwarte, Universität Hamburg, Germany email: uwolter@hs.uni-hamburg.de
Bernhard Aringer
Affiliation:
Dipartimento di Fisica e Astronomia Galileo Galilei, Università di Padova, Italy
Bernd Freytag
Affiliation:
Institutionen för fysik och astronomi, Uppsala Universitet, Sweden
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.

TIGvival is a spectroscopic monitoring program of long-period variables (LPV) using our robotic telescope TIGRE. Since 2013, we obtain low-noise, high-resolution spectra (R= 20 000) that cover the optical regime (3800 Å to 8800 Å). We are now continuously monitoring 7 LPVs with different periods and chemical properties. Our 350+ spectra evenly sample the target cycles, as far as ground-based observations allow. Analyzing the TIGvival spectra of Mira as a sample case, our measurements indicate that the strength of the TiO-absorption is phase-shifted with respect to the visual light curve.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Brand, J., Winnberg, A., Engels, D., 2018, A&A, in preparationGoogle Scholar
Pardo et al. 2004, A&A, 424 145Google Scholar
Reid, M.J. & Goldstone, J.E., 2002, ApJ, 568, 93110.1086/338947CrossRefGoogle Scholar
Tuthill, P.G., Haniff, C.A., & Baldwin, J.E., 1995, MNRAS, 277, 154110.1093/mnras/277.4.1541CrossRefGoogle Scholar
Young et al., 2000, MNRAS, 318, 38110.1046/j.1365-8711.2000.03690.xCrossRefGoogle Scholar