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- Q581019 subject Q1031119.
- Q581019 subject Q10641.
- Q581019 subject Q7215866.
- Q581019 subject Q8335676.
- Q581019 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·s−1. This cluster contains eleven Be stars, two red giants and four Ap stars.".
- Q581019 thumbnail Star_cluster_NGC_3766.jpg?width=300.
- Q581019 wikiPageExternalLink frame_list.cgi?ngc3766.
- Q581019 wikiPageExternalLink n3766.html.
- Q581019 wikiPageExternalLink LambdaCentauri.htm.
- Q581019 wikiPageWikiLink Q102626.
- Q581019 wikiPageWikiLink Q1031119.
- Q581019 wikiPageWikiLink Q10641.
- Q581019 wikiPageWikiLink Q11387.
- Q581019 wikiPageWikiLink Q12129.
- Q581019 wikiPageWikiLink Q14534.
- Q581019 wikiPageWikiLink Q151991.
- Q581019 wikiPageWikiLink Q179600.
- Q581019 wikiPageWikiLink Q202703.
- Q581019 wikiPageWikiLink Q22066400.
- Q581019 wikiPageWikiLink Q2703.
- Q581019 wikiPageWikiLink Q272447.
- Q581019 wikiPageWikiLink Q4213.
- Q581019 wikiPageWikiLink Q459352.
- Q581019 wikiPageWikiLink Q531.
- Q581019 wikiPageWikiLink Q7215866.
- Q581019 wikiPageWikiLink Q8335676.
- Q581019 wikiPageWikiLink Q857461.
- Q581019 wikiPageWikiLink Q8844.
- Q581019 wikiPageWikiLink Q8928.
- Q581019 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.".
- Q581019 label "NGC 3766".
- Q581019 depiction Star_cluster_NGC_3766.jpg.