Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-08T05:03:10.435Z Has data issue: false hasContentIssue false
  • English
  • Français

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 Open the ORCID record for D. M. Bowman [Opens in a new window] ,
B. Vandenbussche ,
H. Sana Open the ORCID record for H. Sana [Opens in a new window] ,
A. Tkachenko ,
G. Raskin ,
T. Delabie ,
B. Vandoren ,
P. Royer ,
S. Garcia Open the ORCID record for S. Garcia [Opens in a new window]  and
T. Van Reeth
...Show all authors
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
*
email: [email protected]
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 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.

Keywords

instrumentation: spectrographsstars: early-typestars: oscillations
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 630 - 632
Check for updates
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

Aerts et al. 1994, A&A, 286, 109 Google Scholar
Briquet et al. 2009, A&A, 506, 269–280 Google Scholar
Bowman et al. 2022, A&A, 658, A96 Google Scholar
Bowman 2020, Frontiers Astron. Space Sci., 7, 70 Google Scholar
Raskin et al. 2018, SPIE proceedings, 10698, id. 106985RGoogle Scholar
Ricker at al. 2015, Astron. Tel. Inst. Sys., 1, 014001 Google Scholar
Supplementary material: PDF

Bowman et al. supplementary material

Bowman et al. supplementary material

Download Bowman et al. supplementary material(PDF)
PDF 4.2 MB