Quantifying Bursty Star Formation in Dwarf Galaxies
Dwarf galaxy star formation histories are theoretically expected to be bursty, potentially leaving distinct imprints on their chemical evolution. We propose that episodic starbursts with quiescent periods longer than ~100 Myr should lead to discontinuous tracks in a dwarf galaxy's [$\alpha$/Fe]...
| 出版年: | The Open Journal of Astrophysics |
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| 主要な著者: | , |
| フォーマット: | 論文 |
| 言語: | 英語 |
| 出版事項: |
Maynooth Academic Publishing
2025-01-01
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| オンライン･アクセス: | https://doi.org/10.33232/001c.128414 |