Low-mass Population III Star Formation due to the HD Cooling Induced by Weak Lyman–Werner Radiation
Lyman–Werner (LW) radiation photodissociating molecular hydrogen (H _2 ) influences the thermal and dynamical evolution of the Population III (Pop III) star-forming gas cloud. The effect of powerful LW radiation has been well investigated in the context of supermassive black hole formation in the ea...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad2fc9 |