Warm Molecular Hydrogen in Nearby, Luminous Infrared Galaxies

Mid-infrared molecular hydrogen (H-2) emission is a powerful cooling agent in galaxy mergers and in radio galaxies; it is a potential key tracer of gas evolution and energy dissipation associated with mergers, star formation, and accretion onto supermassive black holes. We detect mid-IR H-2 line emi...

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Detalles Bibliográficos
Autores principales: Petric, Andreea O., Armus, Lee, Flagey, Nicolas, Guillard, Pierre, Howell, Justin, Inami, Hanae, Charmandaris, Vassillis, Evanss, Aaron, Stierwalt, Sabrina, Diaz-Santos, Tanio, Lu, Nanyao, Spoon, Henrik, Mazzarella, Joe, Appleton, Phil, Chan, Ben, Chu, Jason, Hand, Derek, Privon, George, Sanders, David, Surace, Jason, Xu, Kevin, Zhao, Yinghe
Formato: Artículo (Article)
Idioma:Inglés (English)
Publicado: 2025
Materias:
galaxies: active
galaxies: interactions
galaxies: ISM
galaxies: starburst
Acceso en línea:https://repositorio.uc.cl/handle/11534/101209

Internet

https://repositorio.uc.cl/handle/11534/101209

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