About: V Coronae Australis

An Entity of Type: star, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

V Coronae Australis (V CrA) is a R Coronae Borealis variable star in the constellation Corona Australis. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. V Coronae Australis dimmed in brightness from 1994 to 1998. It has around 60% the mass of the Sun and an effective (surface) temperature of around 6250 K.

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dbo:abstract	V Coronae Australis (V CrA) is a R Coronae Borealis variable star in the constellation Corona Australis. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. V Coronae Australis dimmed in brightness from 1994 to 1998. It has around 60% the mass of the Sun and an effective (surface) temperature of around 6250 K. (en) V Coronae Australis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Södra kronan. Stjärnan har visuell magnitud +9,4 och når i förmörkelsefasen ner till +17,9. V Coronae Australis observerades i förmörkelsefasen från 1994 till 1998. (sv)
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rdfs:comment	V Coronae Australis (V CrA) is a R Coronae Borealis variable star in the constellation Corona Australis. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. V Coronae Australis dimmed in brightness from 1994 to 1998. It has around 60% the mass of the Sun and an effective (surface) temperature of around 6250 K. (en) V Coronae Australis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Södra kronan. Stjärnan har visuell magnitud +9,4 och når i förmörkelsefasen ner till +17,9. V Coronae Australis observerades i förmörkelsefasen från 1994 till 1998. (sv)
rdfs:label	V Coronae Australis (en) V Coronae Australis (sv)
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