Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q5176592> ?p ?o }
Showing triples 1 to 19 of
19
with 100 triples per page.
- Q5176592 subject Q6381547.
- Q5176592 subject Q7009372.
- Q5176592 subject Q8293947.
- Q5176592 subject Q8294236.
- Q5176592 abstract "Lambda Pavonis (λ Pav), also known as HD 173948 or HIP 92609, is a star in the constellation Pavo. Its apparent magnitude is 4.21. It is a Be star, a rapidly rotating hot blue star which has developed a gas disk around it. It is a member of the Scorpius-Centaurus Association. It is a Gamma Cassiopeae variable or shell star which has brightened to magnitude 4.0.Variations in signals coming from Lambda Pavonis have led to debate on whether it is a binary, single or pulsating variable star.".
- Q5176592 wikiPageWikiLink Q10515.
- Q5176592 wikiPageWikiLink Q111130.
- Q5176592 wikiPageWikiLink Q124313.
- Q5176592 wikiPageWikiLink Q179600.
- Q5176592 wikiPageWikiLink Q2288255.
- Q5176592 wikiPageWikiLink Q45059.
- Q5176592 wikiPageWikiLink Q523.
- Q5176592 wikiPageWikiLink Q6381547.
- Q5176592 wikiPageWikiLink Q7009372.
- Q5176592 wikiPageWikiLink Q8293947.
- Q5176592 wikiPageWikiLink Q8294236.
- Q5176592 wikiPageWikiLink Q8928.
- Q5176592 comment "Lambda Pavonis (λ Pav), also known as HD 173948 or HIP 92609, is a star in the constellation Pavo. Its apparent magnitude is 4.21. It is a Be star, a rapidly rotating hot blue star which has developed a gas disk around it. It is a member of the Scorpius-Centaurus Association. It is a Gamma Cassiopeae variable or shell star which has brightened to magnitude 4.0.Variations in signals coming from Lambda Pavonis have led to debate on whether it is a binary, single or pulsating variable star.".
- Q5176592 label "Lambda Pavonis".