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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| Hauptverfasser: | , , , , , , , , , , , , , |
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| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
IOP Publishing
2024-01-01
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| Schriftenreihe: | The Astronomical Journal |
| Schlagworte: | |
| Online-Zugang: | https://doi.org/10.3847/1538-3881/ad7b30 |
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