Matches in DBpedia 2016-04 for { <http://dbpedia.org/resource/OGLE-LMC-CEP0227> ?p ?o }
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- OGLE-LMC-CEP0227 abstract "OGLE-LMC-CEP0227 is an eclipsing binary (Cepheid variable) star, pulsating every 310 days. The star, in the Large Magellanic Cloud, was the first Cepheid star system found to be orbiting exactly edge on.The binary stars orbit each other 'edge on' to the line of sight from the earth. This unique configuration has allowed astronomers to refine their understanding of Cepheid stars. Studies of this very rare system have allowed astronomers to measure the Cepheid mass with unprecedented accuracy. However, study of the stars has indicated that there is still a discrepancy between observed mass and theoretical characteristics of this type of binary star.The two stars orbit each other every 309 days, and each has 4.14 solar masses. The primary component having an effective temperature of 5900k and the secondary a temperature of 5080K.".
- OGLE-LMC-CEP0227 thumbnail Artist’s_impression_of_the_remarkable_double_star_OGLE-LMC-CEP0227.jpg?width=300.
- OGLE-LMC-CEP0227 wikiPageExternalLink 51949650_Is_there_a_mass_discrepancy_in_the_Cepheid_binary_OGLE-LMC-CEP0227.
- OGLE-LMC-CEP0227 wikiPageID "47641692".
- OGLE-LMC-CEP0227 wikiPageLength "2754".
- OGLE-LMC-CEP0227 wikiPageOutDegree "18".
- OGLE-LMC-CEP0227 wikiPageRevisionID "703417728".
- OGLE-LMC-CEP0227 wikiPageWikiLink Astronomer.
- OGLE-LMC-CEP0227 wikiPageWikiLink Binary_star.
- OGLE-LMC-CEP0227 wikiPageWikiLink Category:Astrometry.
- OGLE-LMC-CEP0227 wikiPageWikiLink Category:Classical_Cepheid_variables.
- OGLE-LMC-CEP0227 wikiPageWikiLink Cepheid_variable.
- OGLE-LMC-CEP0227 wikiPageWikiLink Day.
- OGLE-LMC-CEP0227 wikiPageWikiLink Effective_temperature.
- OGLE-LMC-CEP0227 wikiPageWikiLink Kelvin.
- OGLE-LMC-CEP0227 wikiPageWikiLink Large_Magellanic_Cloud.
- OGLE-LMC-CEP0227 wikiPageWikiLink Mass.
- OGLE-LMC-CEP0227 wikiPageWikiLink Orbit.
- OGLE-LMC-CEP0227 wikiPageWikiLink Solar_mass.
- OGLE-LMC-CEP0227 wikiPageWikiLink Star.
- OGLE-LMC-CEP0227 wikiPageWikiLink Star_system.
- OGLE-LMC-CEP0227 wikiPageWikiLink Temperature.
- OGLE-LMC-CEP0227 wikiPageWikiLink File:Artist’s_impression_of_the_remarkable_double_star_OGLE-LMC-CEP0227.jpg.
- OGLE-LMC-CEP0227 wikiPageUsesTemplate Template:Reflist.
- OGLE-LMC-CEP0227 subject Category:Astrometry.
- OGLE-LMC-CEP0227 subject Category:Classical_Cepheid_variables.
- OGLE-LMC-CEP0227 hypernym Star.
- OGLE-LMC-CEP0227 type Star.
- OGLE-LMC-CEP0227 comment "OGLE-LMC-CEP0227 is an eclipsing binary (Cepheid variable) star, pulsating every 310 days. The star, in the Large Magellanic Cloud, was the first Cepheid star system found to be orbiting exactly edge on.The binary stars orbit each other 'edge on' to the line of sight from the earth. This unique configuration has allowed astronomers to refine their understanding of Cepheid stars. Studies of this very rare system have allowed astronomers to measure the Cepheid mass with unprecedented accuracy.".
- OGLE-LMC-CEP0227 label "OGLE-LMC-CEP0227".
- OGLE-LMC-CEP0227 wasDerivedFrom OGLE-LMC-CEP0227?oldid=703417728.
- OGLE-LMC-CEP0227 depiction Artist’s_impression_of_the_remarkable_double_star_OGLE-LMC-CEP0227.jpg.
- OGLE-LMC-CEP0227 isPrimaryTopicOf OGLE-LMC-CEP0227.