About: S Apodis

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

S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. 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. Located around 13,000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K.

Property	Value
dbo:abstract	S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. 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. Located around 13,000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K. (en) S Apodis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Paradisfågeln. Stjärnan har magnitud +9,6 och når i förmörkelsefasen ner till +15,2. (sv)
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rdfs:comment	S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. 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. Located around 13,000 light-years distant, it shines with a luminosity approximately 960 times that of the Sun and has a surface temperature of 3916 K. (en) S Apodis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Paradisfågeln. Stjärnan har magnitud +9,6 och når i förmörkelsefasen ner till +15,2. (sv)
rdfs:label	S Apodis (en) S Apodis (sv)
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