Correlating Intrinsic Stellar Parameters with Mg ii Self-reversal Depths

Correlating Intrinsic Stellar Parameters with Mg ii Self-reversal Depths

The Mg ii h&k emission lines (2803, 2796 Å) are a useful tool for understanding stellar chromospheres and transition regions due to their intrinsic brightness, relatively low interstellar medium (ISM) absorption interference, and abundance of archival spectra available. Similar to other opticall...

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Bibliographic Details
Main Authors: Anna Taylor, Audrey Dunn, Sarah Peacock, Allison Youngblood, Seth Redfield
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Stellar spectral types
Online Access:https://doi.org/10.3847/1538-4357/ad22da

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