α-MC: Self-consistent α-enhanced Stellar Population Models Covering a Wide Range of Age, Metallicity, and Wavelength
We present new stellar population models, α -MC, self-consistently taking into account nonsolar [ α /Fe] abundances for both isochrones and stellar spectra. The α -MC models are based on α -enhanced MIST isochrones and C3K spectral libraries, which are publicly available in FSPS. Our new models cove...
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| Autori principali: | , , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
IOP Publishing
2025-01-01
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| Serie: | The Astrophysical Journal |
| Soggetti: | |
| Accesso online: | https://doi.org/10.3847/1538-4357/ae0cba |
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