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（→特殊恒星） |
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==恒星== |
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*Metallic A stars (Am) Among the A class, the 25% of stars show some oddities. Among all these peculiar stars the most important classes are the metallic A stars (Am)and the magnetic A stars (Ap). |
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Am stars, due to the strong intensity of their metallic lines were first classified in the F class and they were shifted to the A class onlyafter the discovery that their black-body temperature was in the range of the temperatures of A stars. |
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Among the elements that can be found in the atmosphere of these stars with abundancies up to 25 times the average we can find Stronzium,Yttrium, Barium, Zirconium, Zinc and Copper. On the contrary, sole light elements are underabundant, like Calcium and Scandium. |
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===赫罗图=== |
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*基于HST对球状星团 Omega Centauri(半人马座）的观测构建HR图。amazing movie [http://www.spacetelescope.org/videos/heic1017b/] |
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===星震学=== |
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The real physical processes involved in such an odd spectrum were first understood around 1970 when it become clear that Am starsare all unusually slow rotators and that they belong to binary systems where the original fast rotation was slowed down by tidal forcesuntil star rotation was locked with orbital period. |
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*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. |
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Without a fast rotation and without convection that is typical only of colder stars, the atmospheres of these stars are extremely quietand superficial segregation phenomena can arise where the chemical composition is very different from that of deeper layers, producingpeculiar absorption spectra. |
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*可以精确测量log(g),参考[http://arxiv.org/abs/1411.0235] |
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===特殊恒星=== |
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*参考[http://www.astrogeo.va.it/astronom/spettri/apen.htm] |
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*[[Metallic A stars]] (Am) |
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*[[magnetic A stars]] （Ap) |
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*[[BHB stars]] |
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*[[Be star]] |
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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)