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The CubeSpec space mission: Asteroseismology of massive stars from time-series optical spectroscopy

Published online by Cambridge University Press:  29 August 2024

D. M. Bowman*
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
B. Vandenbussche
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
H. Sana
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
A. Tkachenko
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
G. Raskin
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
T. Delabie
Affiliation:
Arcsec NV, Blijde Inkomststraat 22, 3000 Leuven, Belgium
B. Vandoren
Affiliation:
Arcsec NV, Blijde Inkomststraat 22, 3000 Leuven, Belgium
P. Royer
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
S. Garcia
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
T. Van Reeth
Affiliation:
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
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Abstract

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The ESA/KU Leuven CubeSpec mission is specifically designed to provide low-cost space-based high-resolution optical spectroscopy. Here we highlight the science requirements and capabilities of CubeSpec. The primary science goal is to perform pulsation mode identification from spectroscopic line profile variability and empower asteroseismology of massive stars.

Type
Poster Paper
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

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Raskin et al. 2018, SPIE proceedings, 10698, id. 106985RGoogle Scholar
Ricker at al. 2015, Astron. Tel. Inst. Sys., 1, 014001 Google Scholar
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