The Baryonic Tully–Fisher Relation. II. Stellar Mass Models
We present new color–ϒ _* (mass-to-light ratio) models to convert Wide-field Infrared Survey Explorer W1 fluxes into stellar masses. We outline a range of possible star formation histories and chemical evolution scenarios to explore the confidence limits of stellar population models on the value of...
Shranjeno v:
| Principais autores: | , , , |
|---|---|
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2025-01-01
|
| Serija: | The Astronomical Journal |
| Teme: | |
| Online dostop: | https://doi.org/10.3847/1538-3881/adaf21 |
| Oznake: |
Brez oznak, prvi označite!
|