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- NGC_3766 abstract "NGC 3766 is an open star cluster in the southern constellation Centaurus. It is located in the vast star-forming region known as the Carina molecular cloud, and was discovered by Nicolas Louis de Lacaille during his astrometric survey in 1751–1752. At a distance of about 1745 pc, the cluster subtends a diameter of about 12 minutes of arc.There are 137 listed stars, but many are likely non-members, with only 36 have accurate photometric data. Total apparent magnitude of 5.3 and integrated spectral type of B1.7. NGC 3766 is relatively young that is estimated as log (7.160) or 14.4 million years, and approaching us at –14.8 km.sec.−1. This cluster contains eleven Be stars, two red giants and four Ap stars.".
- NGC_3766 thumbnail Star_cluster_NGC_3766.jpg?width=300.
- NGC_3766 wikiPageExternalLink LambdaCentauri.htm.
- NGC_3766 wikiPageExternalLink n3766.html.
- NGC_3766 wikiPageExternalLink frame_list.cgi?ngc3766.
- NGC_3766 wikiPageID "4243413".
- NGC_3766 wikiPageRevisionID "575552057".
- NGC_3766 appmagV "5.3".
- NGC_3766 caption "NGC 3766 image taken with the MPG/ESO 1.2-metre telescope at the La Silla Observatory".
- NGC_3766 constellation Centaurus.
- NGC_3766 credit European_Southern_Observatory.
- NGC_3766 dec "−61° 37′".
- NGC_3766 distLy "5.5".
- NGC_3766 epoch Epoch_(astronomy).
- NGC_3766 hasPhotoCollection NGC_3766.
- NGC_3766 name "NGC 3766".
- NGC_3766 names "Dunlop 289, Melotte 107, Collinder 248, C1133-613, Caldwell 97".
- NGC_3766 names "NGC 3766, Lacaille III.7,".
- NGC_3766 notes "Easy to view via binoculars or telescope".
- NGC_3766 ra "41766.0".
- NGC_3766 sizeV "12".
- NGC_3766 subject Category:Caldwell_objects.
- NGC_3766 subject Category:Centaurus_(constellation).
- NGC_3766 subject Category:NGC_objects.
- NGC_3766 subject Category:Open_clusters.
- NGC_3766 comment "NGC 3766 is an open star cluster in the southern constellation Centaurus. It is located in the vast star-forming region known as the Carina molecular cloud, and was discovered by Nicolas Louis de Lacaille during his astrometric survey in 1751–1752. At a distance of about 1745 pc, the cluster subtends a diameter of about 12 minutes of arc.There are 137 listed stars, but many are likely non-members, with only 36 have accurate photometric data.".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 label "NGC 3766".
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs NGC_3766.
- NGC_3766 sameAs m.0br_fp.
- NGC_3766 sameAs Q581019.
- NGC_3766 sameAs Q581019.
- NGC_3766 wasDerivedFrom NGC_3766?oldid=575552057.
- NGC_3766 depiction Star_cluster_NGC_3766.jpg.
- NGC_3766 isPrimaryTopicOf NGC_3766.