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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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Detalles Bibliográficos
Autores principales:	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.
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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