The Fate of the Interstellar Medium in Early-type Galaxies. V. Active Galactic Nucleus Feedback from Optical Spectral Classification

Quenching of star formation plays a fundamental role in galaxy evolution. This process occurs due to the removal of the cold interstellar medium (ISM) or stabilization against collapse, so that gas cannot be used in the formation of new stars. In this paper, we study the effect of different mechanis...

詳細記述

書誌詳細

出版年:	The Astrophysical Journal Supplement Series
主要な著者:	Oleh Ryzhov, Michał J. Michałowski, J. Nadolny, J. Hjorth, A. Leśniewska, M. Solar, P. Nowaczyk, C. Gall, T. T. Takeuchi
フォーマット:	論文
言語:	英語
出版事項:	IOP Publishing 2025-01-01
主題:	Early-type galaxies Elliptical galaxies Galaxy ages Galaxy evolution Interstellar medium Galaxy quenching
オンライン･アクセス:	https://doi.org/10.3847/1538-4365/ad93cd