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- IC_348 abstract "IC 348 is a star forming region in the constellation Perseus located about 315 parsecs from the Sun. It consists of nebulosity and an associated 2 million year old cluster of roughly 400 stars within an angular diameter of 20″. The most massive stars in the cluster are the binary star system BD+31°643, which has a combined spectral class of B5. Based upon infrared observations using the Spitzer Space Telescope, about half of the stars in the cluster have a circumstellar disk, of which 60% are thick or primordial disks. The age of this cluster has allowed three low mass brown dwarfs to be discovered. These objects lose heat as they age, so they are more readily discovered while they are still young.".
- IC_348 wikiPageExternalLink IC348.html.
- IC_348 wikiPageID "31391131".
- IC_348 wikiPageRevisionID "591760762".
- IC_348 age "6.31152E13".
- IC_348 appmagV "7.3".
- IC_348 caption "Hubble image of IC 348 and its surroundings.".
- IC_348 constellation Perseus_(constellation).
- IC_348 hasPhotoCollection IC_348.
- IC_348 name "IC 348".
- IC_348 names "C 0341+321, Collinder 41".
- IC_348 subject Category:Open_clusters.
- IC_348 comment "IC 348 is a star forming region in the constellation Perseus located about 315 parsecs from the Sun. It consists of nebulosity and an associated 2 million year old cluster of roughly 400 stars within an angular diameter of 20″. The most massive stars in the cluster are the binary star system BD+31°643, which has a combined spectral class of B5.".
- IC_348 label "IC 348".
- IC_348 label "IC 348".
- IC_348 label "IC 348".
- IC_348 label "IC 348".
- IC_348 sameAs IC_348.
- IC_348 sameAs IC_348.
- IC_348 sameAs m.0gkz4vc.
- IC_348 sameAs Q645964.
- IC_348 sameAs Q645964.
- IC_348 wasDerivedFrom IC_348?oldid=591760762.
- IC_348 isPrimaryTopicOf IC_348.