“天文基础知识”的版本间差异
跳到导航
跳到搜索
无编辑摘要 |
（→特殊恒星） |
||
| （未显示同一用户的1个中间版本） | |||
| 第7行： | 第7行： | ||
*Asteroseismology (from Greek ἀστήρ, astēr, "star"; σεισμός, seismos, "earthquake"; and -λογία, -logia) also known as stellar seismology[1][2] is the science that studies the internal structure of pulsating stars by the interpretation of their frequency spectra. |
*Asteroseismology (from Greek ἀστήρ, astēr, "star"; σεισμός, seismos, "earthquake"; and -λογία, -logia) also known as stellar seismology[1][2] is the science that studies the internal structure of pulsating stars by the interpretation of their frequency spectra. |
||
*可以精确测量log(g) |
*可以精确测量log(g),参考[http://arxiv.org/abs/1411.0235] |
||
===特殊恒星=== |
===特殊恒星=== |
||
| 第17行： | 第17行： | ||
*[[BHB stars]] |
*[[BHB stars]] |
||
*[[Be star]] |
|||
2014年12月13日 (六) 08:50的最新版本
恒星
赫罗图
- 基于HST对球状星团 Omega Centauri(半人马座）的观测构建HR图。amazing movie [1]
星震学
- Asteroseismology (from Greek ἀστήρ, astēr, "star"; σεισμός, seismos, "earthquake"; and -λογία, -logia) also known as stellar seismology[1][2] is the science that studies the internal structure of pulsating stars by the interpretation of their frequency spectra.
- 可以精确测量log(g),参考[2]
特殊恒星
- 参考[3]
- Metallic A stars (Am)
- magnetic A stars （Ap)