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- Omega_Centauri abstract "Omega Centauri (ω Cen) or NGC 5139, is a globular clusterin the constellation of Centaurus that was discovered by Edmond Halley in 1677. Located at a distance of 15,800 light-years (4,850 pc), it is the largest globular cluster in the Milky Way galaxy. Omega Centauri is so distinctive from the other galactic globular clusters that it is thought to have an alternate origin as the core remnant of a disrupted dwarf galaxy.".
- Omega_Centauri thumbnail Omega_Centauri_by_ESO.jpg?width=300.
- Omega_Centauri wikiPageExternalLink factsheet.php?p=omega-centauri.
- Omega_Centauri wikiPageExternalLink cluster_4.php?ggc=Omega+Cen.
- Omega_Centauri wikiPageExternalLink a.
- Omega_Centauri wikiPageExternalLink media_release_030716.php.
- Omega_Centauri wikiPageExternalLink bi2410.shtml.
- Omega_Centauri wikiPageExternalLink opo0133a.html.
- Omega_Centauri wikiPageExternalLink ?ra=13.44057&de=-47.482835&zoom=9&img_source=IMG_1403:all.
- Omega_Centauri wikiPageID "914432".
- Omega_Centauri wikiPageRevisionID "601680065".
- Omega_Centauri age "11.52".
- Omega_Centauri appmagV "3.9".
- Omega_Centauri caption "The globular cluster Omega Centauri. Credit ESO".
- Omega_Centauri class "VIII".
- Omega_Centauri constellation Centaurus.
- Omega_Centauri epoch Epoch_(astronomy).
- Omega_Centauri hasPhotoCollection Omega_Centauri.
- Omega_Centauri metalFe "–1.35".
- Omega_Centauri name "Omega Centauri".
- Omega_Centauri names "NGC 5139, GCl 24, ω Centauri, Caldwell 80".
- Omega_Centauri radiusLy "86".
- Omega_Centauri sizeV "36".
- Omega_Centauri subject Category:Bayer_objects.
- Omega_Centauri subject Category:Caldwell_objects.
- Omega_Centauri subject Category:Centaurus_(constellation).
- Omega_Centauri subject Category:Globular_clusters.
- Omega_Centauri subject Category:NGC_objects.
- Omega_Centauri type BayerObjects.
- Omega_Centauri type CaldwellObjects.
- Omega_Centauri type NGCObjects.
- Omega_Centauri type Object100002684.
- Omega_Centauri type PhysicalEntity100001930.
- Omega_Centauri comment "Omega Centauri (ω Cen) or NGC 5139, is a globular clusterin the constellation of Centaurus that was discovered by Edmond Halley in 1677. Located at a distance of 15,800 light-years (4,850 pc), it is the largest globular cluster in the Milky Way galaxy. Omega Centauri is so distinctive from the other galactic globular clusters that it is thought to have an alternate origin as the core remnant of a disrupted dwarf galaxy.".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Omega Centauri".
- Omega_Centauri label "Ω星団".
- Omega_Centauri label "Омега Центавра".
- Omega_Centauri label "半人马座ω".
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Ω星団.
- Omega_Centauri sameAs 오메가_성단.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri sameAs m.03pg1t.
- Omega_Centauri sameAs Q14275.
- Omega_Centauri sameAs Q14275.
- Omega_Centauri sameAs Omega_Centauri.
- Omega_Centauri wasDerivedFrom Omega_Centauri?oldid=601680065.
- Omega_Centauri depiction Omega_Centauri_by_ESO.jpg.
- Omega_Centauri isPrimaryTopicOf Omega_Centauri.
