BPM 37093
1. V886 CentauriV886 Centauri (BPM 37093) is a variable white dwarf star of the DAV, or ZZ Ceti, type, with a hydrogen atmosphere and an unusually high mass of approximately 1.1 times the Sun's. It is about 50 light-years from Earth, in the constellation Centaurus, and vibrates; these pulsations cause its luminosity to vary. Like other white dwarfs, V886 Centauri is thought to be composed primarily of carbon and oxygen, which are created by thermonuclear fusion of helium nuclei in the triple-alpha process.
Read “V886 Centauri” on English Wikipedia
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Read “V886 Centauri” on DBpedia
Read “V886 Centauri” on English Wikipedia
Read “BPM 37093” on Japanese Wikipedia
Read “V886 Centauri” on DBpedia
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