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Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities

Fuente: arXiv

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Bibliographic Details
Main Authors:	Cleri, Nikko J., Olivier, Grace M., Backhaus, Bren E., Leja, Joel, Papovich, Casey, Trump, Jonathan R., Haro, Pablo Arrabal, Buat, Veronique, Burgarella, Denis, Burnham, Emilie, Calabro, Antonello, Cohn, Jonathan H., Cole, Justin W., Davis, Kelcey, Dickinson, Mark, Finkelstein, Steven L., Garner III, Ray, Hirschmann, Michaela, Hu, Weida, Hutchison, Taylor A., Kocevski, Dale D., Koekemoer, Anton M., Larson, Rebecca L., Lewis, Zach J., Maseda, Michael V., Seille, Lise-Marie, Simons, Raymond C.
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2506.21660