Post-AGB Binaries as Interacting Systems

doi:10.3390-galaxies13030068

2025-08-21

PRE

H. Van Winckel

DOI：10.3390-galaxies13030068

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我们介绍了关于低至中等初始质量演化双星中起作用的物理相互作用机制的最新研究进展，这些双星被稳定的气体和尘埃盘包围。这些系统被称为渐近巨星支后（post-AGB）双星，但最近研究表明，其中一些系统的光度过低，应被视为红巨星支后（post-RGB）系统。尽管这些系统目前完全处于洛希瓣内，但它们仍显示出不同组成部分之间存在活跃且持续的相互作用迹象。我们以一些未来研究计划作为本贡献的结尾。

Keyword:

post-AGB binaries

post-RGB binaries

evolved binaries

disc interaction

stellar evolution

期刊

Galaxies

IF:

3.8

论文数:

826

被引数:

2.1K

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