方法证据记录
Stellar Population Synthesis
Stellar population synthesis is a technique for modeling the integrated light from a galaxy by summing the contributions of all individual stars formed at different times and with different masses and metallicities. Developed systematically by Bruzual and Charlot (2003), this approach enables estimation of fundamental galaxy properties from observations without detailed knowledge of individual stars.
源记录
引文逐字复制自方法源记录。这些引文不代表任何层级的验证。
Stellar Population Synthesis Models for Galaxy Evolution
分类方法记录 · process-pipeline / astronomy
- Bruzual, G., & Charlot, S. (2003). Stellar population synthesis at arbitrary metallicity with the Bruzual & Charlot models. Monthly Notices of the Royal Astronomical Society, 344(3), 1000-1028. · DOI 10.1046/j.1365-8711.2003.06897.x
- Charlot, S., & Fall, S. M. (1995). Dust-free star formation histories of galaxies: consequences for age dating and extinction measurements. Astrophysical Journal, 539(2), 718-730. · URL
- Conroy, C., Gunn, J. E., & White, M. (2013). The propagation of uncertainties in stellar population synthesis modeling. Astrophysical Journal, 414(2), 184-207. · URL
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