arXiv Open Access 2024

Methods to Characterise Exoplanet Host Stars from Spectroscopy

Carina M. Persson
Lihat Sumber

Abstrak

A key to understand exoplanets is characterisation of their host stars. One of the most powerful tools to characterise stellar properties like effective temperature, surface gravity and metallicity, is spectroscopy based on observations of stellar atmospheres. This chapter describes the stellar parameters that can be derived from a spectrum with examples of well established methods and theoretical model atmospheres. Combined with photometry and parallax measurements, the outcome of the spectroscopic modelling can be used to derive stellar radii and masses.

Topik & Kata Kunci

Penulis (1)

C

Carina M. Persson

Format Sitasi

Persson, C.M. (2024). Methods to Characterise Exoplanet Host Stars from Spectroscopy. https://arxiv.org/abs/2411.19306

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓