The FUor Mass Distribution Matches the Solar Neighborhood Initial Mass Function: Evidence for a Universal Eruptive Phase
Eruptive accretion events are expected to play an important role in the mass-buildup stage of individual star formation. FU Ori objects (FUors) experience the most extreme eruptive outbursts, which raise the accretion rate of the disk from 10 ^−9 –10 ^−8 to 10 ^−5 –10 ^−4 M _⊙ yr ^−1 and last for de...
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| Κύριοι συγγραφείς: | , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
IOP Publishing
2026-01-01
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| Σειρά: | The Astrophysical Journal |
| Θέματα: | |
| Διαθέσιμο Online: | https://doi.org/10.3847/1538-4357/ae710e |
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