Why Are Optical Coronal Lines Faint in Active Galactic Nuclei?. McKaig, J. D., Satyapal, S., Laor, A., Abel, N. P., Doan, S. M., Ricci, C., & Cann, J. M. \apj, 976(1):130, November, 2024. doi bibtex @ARTICLE{2024ApJ...976..130M,
author = {{McKaig}, Jeffrey D. and {Satyapal}, Shobita and {Laor}, Ari and {Abel}, Nicholas P. and {Doan}, Sara M. and {Ricci}, Claudio and {Cann}, Jenna M.},
title = "{Why Are Optical Coronal Lines Faint in Active Galactic Nuclei?}",
journal = {\apj},
keywords = {Active galaxies, Quasars, Line intensities, 17, 1319, 2084, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena},
year = 2024,
month = nov,
volume = {976},
number = {1},
eid = {130},
pages = {130},
doi = {10.3847/1538-4357/ad7a79},
archivePrefix = {arXiv},
eprint = {2408.15229},
primaryClass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2024ApJ...976..130M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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