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- Cl*_1806-20 abstract "Cl* 1806-20 is a heavily obscured star cluster on the far side of the Milky Way Galaxy, approximately 50,000 light years distant. It contains the Soft Gamma-Ray Repeater SGR 1806-20 and the luminous blue variable hypergiant star LBV 1806-20, a candidate for the most luminous star in the Galaxy. LBV 1806-20 and many of the other massive stars in the cluster are believed likely to end as supernovas in a few million years, leaving only neutron stars or black holes as remnants.The cluster is heavily obscured by intervening dust, and mostly visible in the infrared.It is part of the larger W31 H II region and giant molecular cloud.It has a compact core (diam ~0.2 pc) with a more extended halo (diam ~2 pc) containing the LBV, and also contains at least three Wolf-Rayet stars (of types WC8, WN6, and WN7) and an OB supergiant, plus other young massive stars.".
- Cl*_1806-20 wikiPageExternalLink 850.htm.
- Cl*_1806-20 wikiPageID "17914618".
- Cl*_1806-20 wikiPageLength "1937".
- Cl*_1806-20 wikiPageOutDegree "24".
- Cl*_1806-20 wikiPageRevisionID "702693379".
- Cl*_1806-20 wikiPageWikiLink Black_hole.
- Cl*_1806-20 wikiPageWikiLink Category:Open_clusters.
- Cl*_1806-20 wikiPageWikiLink Category:Sagittarius_(constellation).
- Cl*_1806-20 wikiPageWikiLink H_II_region.
- Cl*_1806-20 wikiPageWikiLink Hypergiant.
- Cl*_1806-20 wikiPageWikiLink Infrared_astronomy.
- Cl*_1806-20 wikiPageWikiLink LBV_1806-20.
- Cl*_1806-20 wikiPageWikiLink Luminous_blue_variable.
- Cl*_1806-20 wikiPageWikiLink Milky_Way.
- Cl*_1806-20 wikiPageWikiLink Molecular_cloud.
- Cl*_1806-20 wikiPageWikiLink Neutron_star.
- Cl*_1806-20 wikiPageWikiLink SGR_1806-20.
- Cl*_1806-20 wikiPageWikiLink Soft_gamma_repeater.
- Cl*_1806-20 wikiPageWikiLink Star_cluster.
- Cl*_1806-20 wikiPageWikiLink Supernova.
- Cl*_1806-20 wikiPageWikiLink Wolf–Rayet_star.
- Cl*_1806-20 wikiPageWikiLinkText "Cl* 1806-20".
- Cl*_1806-20 wikiPageWikiLinkText "cluster 1806-20".
- Cl*_1806-20 constellation "Sagittarius".
- Cl*_1806-20 distLy "~50000 ly".
- Cl*_1806-20 distPc "~15000 pc".
- Cl*_1806-20 epoch "2000".
- Cl*_1806-20 name "Cl* 1806-20".
- Cl*_1806-20 names "G10.0-0.3, W31".
- Cl*_1806-20 notes "Contains SGR 1806-20 and LBV 1806-20.".
- Cl*_1806-20 wikiPageUsesTemplate Template:DEC.
- Cl*_1806-20 wikiPageUsesTemplate Template:Infobox_Cluster.
- Cl*_1806-20 wikiPageUsesTemplate Template:RA.
- Cl*_1806-20 wikiPageUsesTemplate Template:Reflist.
- Cl*_1806-20 wikiPageUsesTemplate Template:Star-cluster-stub.
- Cl*_1806-20 subject Category:Open_clusters.
- Cl*_1806-20 subject Category:Sagittarius_(constellation).
- Cl*_1806-20 comment "Cl* 1806-20 is a heavily obscured star cluster on the far side of the Milky Way Galaxy, approximately 50,000 light years distant. It contains the Soft Gamma-Ray Repeater SGR 1806-20 and the luminous blue variable hypergiant star LBV 1806-20, a candidate for the most luminous star in the Galaxy.".
- Cl*_1806-20 label "Cl* 1806-20".
- Cl*_1806-20 sameAs Q5177648.
- Cl*_1806-20 sameAs 1806-20.
- Cl*_1806-20 sameAs 성단_1806-20.
- Cl*_1806-20 sameAs Cl*_1806-20.
- Cl*_1806-20 sameAs m.047tccm.
- Cl*_1806-20 sameAs Q5177648.
- Cl*_1806-20 wasDerivedFrom Cl*_1806-20?oldid=702693379.
- Cl*_1806-20 isPrimaryTopicOf Cl*_1806-20.