Thomas Bensby
Senior lecturer
The discovery space of ELT-ANDES. Stars and stellar populations
Author
Summary, in English
The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is the optical and near-infrared high-resolution echelle spectrograph envisioned for the Extremely Large Telescope (ELT). We present a selection of science cases, supported by new calculations and simulations, where ANDES could enable major advances in the fields of stars and stellar populations. We focus on three key areas, including the physics of stellar atmospheres, structure, and evolution; stars of the Milky Way, Local Group, and beyond; and the star-planet connection. The key features of ANDES are its wide wavelength coverage at high spectral resolution and its access to the large collecting area of the ELT. These features position ANDES to address the most compelling questions and potentially transformative advances in stellar astrophysics of the decades ahead, including questions which cannot be anticipated today.
Department/s
- Astrophysics
Publishing year
2024-04
Language
English
Publication/Series
Experimental Astronomy
Volume
57
Issue
2
Document type
Journal article
Publisher
Springer
Topic
- Astronomy, Astrophysics and Cosmology
Keywords
- Galactic archaeology (2178)
- High resolution spectroscopy (2096)
- Star clusters (1567)
- Stellar atmospheres (1584)
- Stellar evolution (1599)
- Stellar physics (1621)
- Stellar populations (1622)
Status
Published
ISBN/ISSN/Other
- ISSN: 0922-6435