Probing Heavily Obscured Active Galactic Nuclei in Major Galaxy Mergers Using the Millimeter–X-Ray Correlation

The study of heavily obscured supermassive black hole (SMBH) growth in late-stage galaxy mergers is challenging: column densities N _H > 10 ^24 cm ^−2 can block most nuclear emission, leaving significant gaps in the SMBH growth census. Millimeter-wave continuum emission offers a potential window int...

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Xehetasun bibliografikoak

Egile Nagusiak:	Macarena Droguett-Callejas, Ezequiel Treister, Loreto Barcos-Muñoz, Makoto Johnstone, Franz E. Bauer, Taiki Kawamuro, Núria Torres-Albà, Claudio Ricci, Michael Koss, Yiqing Song, Alessandro Peca, Aaron Evans, Jorge González
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2026-01-01
Saila:	The Astrophysical Journal Letters
Gaiak:	Supermassive black holes AGN host galaxies Millimeter astronomy Active galactic nuclei
Sarrera elektronikoa:	https://doi.org/10.3847/2041-8213/ae4008
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