Measuring Sub-Kelvin Variations in Stellar Temperature with High-resolution Spectroscopy

The detection of stellar variability often relies on the measurement of selected activity indicators, such as coronal emission lines and nonthermal emissions. On the flip side, the effective stellar temperature is normally seen as one of the key fundamental parameters (with mass and radius) to under...

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Bibliografski detalji

Glavni autori:	Étienne Artigau, Charles Cadieux, Neil J. Cook, René Doyon, Laurie Dauplaise, Luc Arnold, Maya Cadieux, Jean-François Donati, Paul Cristofari, Xavier Delfosse, Pascal Fouqué, Claire Moutou, Pierre Larue, Romain Allart
Format:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2024-01-01
Serija:	The Astronomical Journal
Teme:	Stellar effective temperatures High resolution spectroscopy Time series analysis
Online pristup:	https://doi.org/10.3847/1538-3881/ad7b30
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