About: WR 120

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

WR 120 is a binary containing two Wolf-Rayet stars in the constellation of Scutum, around 10,000 light years away. The primary is a hydrogen-free weak-lined WN7 star, the secondary is a hydrogen-free WN3 or 4 star, and the system is a possible member of the cluster Dolidze 33. From our point of view, WR 120 is reddened by 4.82 magnitudes, and it has the variable designation of V462 Scuti.

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dbo:abstract
  • WR 120 is a binary containing two Wolf-Rayet stars in the constellation of Scutum, around 10,000 light years away. The primary is a hydrogen-free weak-lined WN7 star, the secondary is a hydrogen-free WN3 or 4 star, and the system is a possible member of the cluster Dolidze 33. From our point of view, WR 120 is reddened by 4.82 magnitudes, and it has the variable designation of V462 Scuti. (en)
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  • −3.81 (en)
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  • 1.040000 (xsd:double)
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  • WN7w + WN3/4 (en)
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dbp:epoch
  • J2000 (en)
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  • 83200 (xsd:integer)
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  • 7 (xsd:integer)
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  • 0.054100 (xsd:double)
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  • 0.324600 (xsd:double)
dbp:propMoDec
  • −2.524 (en)
dbp:propMoRa
  • −0.489 (en)
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  • WR 120 is a binary containing two Wolf-Rayet stars in the constellation of Scutum, around 10,000 light years away. The primary is a hydrogen-free weak-lined WN7 star, the secondary is a hydrogen-free WN3 or 4 star, and the system is a possible member of the cluster Dolidze 33. From our point of view, WR 120 is reddened by 4.82 magnitudes, and it has the variable designation of V462 Scuti. (en)
rdfs:label
  • WR 120 (en)
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  • WR 120 (en)
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