Pulsational Mass Loss from Supermassive Stars Creates the Compact Shells of Little Red Dots
Little Red Dots (LRDs) have emerged as one of the central puzzles of the JWST era. Their spectra increasingly require dense gas close to the source, yet the physical origin of that cocoon-like structure remains unclear. We examine whether late pulsational mass loss from supermassive stars (SMSs) lea...
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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
2026-01-01
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| シリーズ: | The Astrophysical Journal Letters |
| 主題: | |
| オンライン･アクセス: | https://doi.org/10.3847/2041-8213/ae82f3 |
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