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- Q18210648 subject Q7215988.
- Q18210648 subject Q8334040.
- Q18210648 subject Q8617505.
- Q18210648 subject Q8691170.
- Q18210648 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 Borealis 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.".
- Q18210648 wikiPageWikiLink Q10413.
- Q18210648 wikiPageWikiLink Q143003.
- Q18210648 wikiPageWikiLink Q1666400.
- Q18210648 wikiPageWikiLink Q2703.
- Q18210648 wikiPageWikiLink Q555846.
- Q18210648 wikiPageWikiLink Q593448.
- Q18210648 wikiPageWikiLink Q7215988.
- Q18210648 wikiPageWikiLink Q8334040.
- Q18210648 wikiPageWikiLink Q854050.
- Q18210648 wikiPageWikiLink Q8617505.
- Q18210648 wikiPageWikiLink Q8691170.
- Q18210648 wikiPageWikiLink Q8928.
- Q18210648 wikiPageWikiLink Q920941.
- Q18210648 type Place.
- Q18210648 type CelestialBody.
- Q18210648 type Location.
- Q18210648 type Place.
- Q18210648 type Star.
- Q18210648 type Thing.
- Q18210648 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 Borealis 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.".
- Q18210648 label "V Coronae Australis".
- Q18210648 name "V Coronae Australis".