PHANGS-ML: The Universal Relation between PAH Band and Optical Line Ratios across Nearby Star-forming Galaxies

The structure and chemistry of the dusty interstellar medium (ISM) are shaped by complex processes that depend on the local radiation field, gas composition, and dust grain properties. Of particular importance are polycyclic aromatic hydrocarbons (PAHs), which emit strong vibrational bands in the mi...

ver descrição completa

Detalhes bibliográficos

Principais autores:	Dalya Baron, Karin M. Sandstrom, Jessica Sutter, Hamid Hassani, Brent Groves, Adam K. Leroy, Eva Schinnerer, Médéric Boquien, Matilde Brazzini, Jérémy Chastenet, Daniel A. Dale, Oleg V. Egorov, Simon C. O. Glover, Ralf S. Klessen, Debosmita Pathak, Erik Rosolowsky, Frank Bigiel, Mélanie Chevance, Kathryn Grasha, Annie Hughes, J. Eduardo Méndez-Delgado, Jérôme Pety, Thomas G. Williams, Stephen Hannon, Sumit K. Sarbadhicary
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal
Assuntos:	Interstellar medium Warm ionized medium Interstellar dust Polycyclic aromatic hydrocarbons Astrostatistics
Acesso em linha:	https://doi.org/10.3847/1538-4357/ad972a
Tags:	Adicionar Tag Sem tags, seja o primeiro a adicionar uma tag!