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...
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| 主要な著者: | , , , , , , , , |
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| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
IOP Publishing
2025-01-01
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| シリーズ: | The Astrophysical Journal Supplement Series |
| 主題: | |
| オンライン･アクセス: | https://doi.org/10.3847/1538-4365/ad93cd |
| タグ: |
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