Disentangling age and metallicity in distant unresolved stellar systems

M. Cantiello, E. Brocato, G.Raimondo
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Abstract

We present some results of an observational and theoretical study on unresolved stellar systems based on the Surface Brightness Fluctuations (SBF) technique. It is shown that SBF magnitudes are a valuable tracer of stellar population properties, and a reliable distance indicator. SBF magnitudes, SBF‐colors, and SBF‐gradients can help to constrain within relatively narrow limits the metallicity and age of the dominant stellar component in distant stellar systems, especially if coupled with other spectro‐photometric indicators.
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解开遥远未解恒星系统中年龄和金属丰度的纠缠
本文介绍了基于表面亮度波动(SBF)技术对未解析恒星系统的观测和理论研究的一些结果。结果表明,SBF星等是一种有价值的恒星星族性质的示踪剂,也是一种可靠的距离指示器。SBF星等、SBF颜色和SBF梯度可以帮助将遥远恒星系统中主要恒星成分的金属丰度和年龄限制在相对狭窄的范围内,特别是如果与其他光谱光度指标相结合的话。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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