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About: UGC 6093

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

UGC 6093 is a barred spiral galaxy located approximately 500 million light years (or about 153 megaparsecs) away from Earth in the constellation of Leo. This galaxy is known to host an active galactic nucleus, which is caused by the accretion of matter by a supermassive black hole located at its center, thus causing it to emit huge amounts of radiation and making UGC 6093's core shine excessively. This galaxy is also a megamaser, which means that it acts as a giant astronomical laser generating microwaves rather than visible light.

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dbo:abstract
  • UGC 6093 is a barred spiral galaxy located approximately 500 million light years (or about 153 megaparsecs) away from Earth in the constellation of Leo. This galaxy is known to host an active galactic nucleus, which is caused by the accretion of matter by a supermassive black hole located at its center, thus causing it to emit huge amounts of radiation and making UGC 6093's core shine excessively. This galaxy is also a megamaser, which means that it acts as a giant astronomical laser generating microwaves rather than visible light. (en)
  • UGC 6093是一个棒旋星系，距离地球约5亿光年（或153百万秒差距）远，坐落于狮子座中。 这个星系是已知的活动星系核的宿主星系，活动星系核是由星系中心的超大质量黑洞对物质吸积而产生的，因而导致它散发巨量的电磁辐射，使得UGC 6093的核心过量发光。该星系也是一个，这意味着它表现得像天文学激光激发器，产生微波，而不是可见光。 (zh)
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  • 2603 (xsd:nonNegativeInteger)
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  • 1023625017 (xsd:integer)
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  • 14.700000 (xsd:double)
dbp:caption
  • Hubble Space Telescope image of UGC 6093 (en)
dbp:constellationName
dbp:distLy
  • 500 (xsd:integer)
dbp:epoch
dbp:hRadialV
  • 10828.0
dbp:imageSize
  • 250 (xsd:integer)
dbp:name
  • UGC 6093 (en)
dbp:names
  • MCG+02-28-044, PGC 33198 (en)
dbp:notes
  • Acts as a megamaser, hosts an AGN. (en)
dbp:pgc
  • 33198 (xsd:integer)
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  • 0.940000 (xsd:double)
dbp:type
  • SABbc (en)
dbp:ugc
  • 6093 (xsd:integer)
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  • 0.036118 (xsd:double)
dcterms:subject
rdf:type
rdfs:comment
  • UGC 6093 is a barred spiral galaxy located approximately 500 million light years (or about 153 megaparsecs) away from Earth in the constellation of Leo. This galaxy is known to host an active galactic nucleus, which is caused by the accretion of matter by a supermassive black hole located at its center, thus causing it to emit huge amounts of radiation and making UGC 6093's core shine excessively. This galaxy is also a megamaser, which means that it acts as a giant astronomical laser generating microwaves rather than visible light. (en)
  • UGC 6093是一个棒旋星系，距离地球约5亿光年（或153百万秒差距）远，坐落于狮子座中。 这个星系是已知的活动星系核的宿主星系，活动星系核是由星系中心的超大质量黑洞对物质吸积而产生的，因而导致它散发巨量的电磁辐射，使得UGC 6093的核心过量发光。该星系也是一个，这意味着它表现得像天文学激光激发器，产生微波，而不是可见光。 (zh)
rdfs:label
  • UGC 6093 (en)
  • UGC 6093 (zh)
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foaf:depiction
foaf:isPrimaryTopicOf
foaf:name
  • MCG+02-28-044,PGC 33198 (en)
  • UGC6093 (en)
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