吸积理论 [
xī jī lǐ lùn]
accretion theory
- 中文摘要1980年代之后,不论是理论天文学家或是观测天文学家,对矮新星中吸积盘的不稳定性都很有兴趣。
After 1980s, the instabilities of accretion discs in dwarf novae interest both theoreticians and observers very much. - 虽然研究人员尚未完全解决这个争论,但多数认为连续吸积学说是两者之中较可行的理论。我将在这里探讨此学说。
Although researchers have not settled this controversy, most consider the sequential-accretion scenario the most plausible of the two. I will focus on it here.
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