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整合恒星群的无处不在时间变化
Charlie Conroy1, Pieter G van Dokkum2, Jieun Choi1
1Department of Astronomy, Harvard University, Cambridge, Massachusetts, USA.
长周期变星,对恒星进化至关重要,展示
科学领域:
- 天文学与天体物理学
- 恒星进化
背景情况:
- 长周期变星代表恒星进化的一个晚期阶段 (非对称巨星分支).
- 它们的脉冲周期对恒星年龄敏感,但由于质量损失和混合不确定性,它们的寿命受到很小的限制.
- 以前的星系光谱能量分布模型没有考虑这些恒星的时间变化.
研究的目的:
- 开发具有长周期变星的依赖时间的恒星群体模型.
- 研究这些变星对星系建模的影响.
- 为了检测和描述星系中预测的"像素闪".
主要方法:
- 构建时间依赖的恒星人口合成模型.
- 在模型中包含长期变星效应.
- 观测和分析银河系M87的像素光曲线.
主要成果:
- 在巨大的金属丰富的星系M87中检测到无处不在的"像素闪".
- 观察到的光曲线变化 (0.11%) 与模型预测密切匹配.
- 与当前的恒星进化模型相比,推断M87的长周期变量寿命缩短了30%.
结论:
- 时间依赖模型准确地捕捉了长周期变星的变性.
- "像素闪"是可以在老,富含金属的恒星群体中检测到的现象.
- 恒星进化模型需要对长期变量恒星寿命进行细化.
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