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・ Helium atom scattering
・ Helium Comedy Club
・ Helium cryogenics
・ Helium dating
・ Helium dilution technique
・ Helium dimer
・ Helium flash
・ Helium focusing cone
・ Helium hydride ion
・ Helium ionization detector
・ Helium line ratio
・ Helium mass spectrometer
・ Helium planet
・ Helium production in the United States
・ Helium release valve
Helium star
・ Helium trimer
・ Helium Vola
・ Helium Vola (album)
・ Helium-3
・ Helium-3 refrigerator
・ Helium-3 surface spin echo
・ Helium-4
・ Helium.com
・ HeliumV
・ Helium–neon laser
・ Heliura
・ Heliura amazonicum
・ Heliura assimilis
・ Heliura baleris


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Helium star : ウィキペディア英語版
Helium star
A helium star or helium strong star is a class O or B star (blue), which has extraordinarily strong helium lines and weaker than normal hydrogen lines, indicating strong stellar winds and a mass loss of the outer envelope. ''Extreme helium stars'' (EHe) entirely lack hydrogen in their spectra.〔(Daviddarling.info: helium star )〕
Previously, a ''helium star'' was a synonym for a B class star, but this usage is considered obsolete.
A ''helium star'' is also a term for a hypothetical star that could occur if two helium white dwarfs with a combined mass of at least 0.5 solar masses merge and subsequently start nuclear fusion of helium, with a lifetime of a few hundred million years. It is believed this is the origin of the extreme helium stars.
==See also==

* R Coronae Borealis variable

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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