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...

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書誌詳細

出版年:	The Astrophysical Journal
主要な著者:	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
フォーマット:	論文
言語:	英語
出版事項:	IOP Publishing 2025-01-01
主題:	Interstellar medium Warm ionized medium Interstellar dust Polycyclic aromatic hydrocarbons Astrostatistics
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/ad972a