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- NGC_3077 abstract "NGC 3077 is a smaller member of the M81 Group. It looks much like an elliptical galaxy. However, it is peculiar for two reasons. First, it shows wispy edges and scattered dust clouds that are probably a result of gravitational interaction with its larger neighbors, similar to the galaxy M82. Second, this galaxy has an active nucleus. This caused Carl Seyfert in 1943 to include it in his list of galaxies, which are now called Seyfert Galaxies. However, NGC 3077, though an emission line galaxy, is today no longer classified as a Seyfert galaxy. NGC 3077 was discovered by William Herschel on November 8, 1801. He remarked that "On the nF (NE) side, there is a faint ray interrupting the roundness." Admiral Smyth described it as "A bright-class round nebula; it is a lucid white, and lights up in the centre ... between these [stars,] the sky is intensely black, and shows the nebula as if floating in awful and illimitable space, at an inconceivable distance."".
- NGC_3077 thumbnail NGC_3077_Hubble.jpg?width=300.
- NGC_3077 wikiPageExternalLink n3077.html.
- NGC_3077 wikiPageID "3876919".
- NGC_3077 wikiPageRevisionID "539756158".
- NGC_3077 appmagV "10.6".
- NGC_3077 caption "NGC 3077 by HST, 1.5′ view".
- NGC_3077 constellationName Ursa_Major.
- NGC_3077 distLy "12.8".
- NGC_3077 epoch Epoch_(astronomy).
- NGC_3077 hasPhotoCollection NGC_3077.
- NGC_3077 name "NGC 3077".
- NGC_3077 names "UGC 5398, PGC 29146".
- NGC_3077 sizeV "5".
- NGC_3077 type "I0 pec".
- NGC_3077 z "14".
- NGC_3077 subject Category:Irregular_galaxies.
- NGC_3077 subject Category:M81_Group.
- NGC_3077 subject Category:NGC_objects.
- NGC_3077 subject Category:PGC_objects.
- NGC_3077 subject Category:Peculiar_galaxies.
- NGC_3077 subject Category:UGC_objects.
- NGC_3077 subject Category:Ursa_Major_(constellation).
- NGC_3077 type CelestialBody.
- NGC_3077 type Galaxy.
- NGC_3077 type PhysicalBody.
- NGC_3077 comment "NGC 3077 is a smaller member of the M81 Group. It looks much like an elliptical galaxy. However, it is peculiar for two reasons. First, it shows wispy edges and scattered dust clouds that are probably a result of gravitational interaction with its larger neighbors, similar to the galaxy M82. Second, this galaxy has an active nucleus. This caused Carl Seyfert in 1943 to include it in his list of galaxies, which are now called Seyfert Galaxies.".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 label "NGC 3077".
- NGC_3077 sameAs NGC_3077.
- NGC_3077 sameAs NGC_3077.
- NGC_3077 sameAs NGC_3077.
- NGC_3077 sameAs NGC_3077.
- NGC_3077 sameAs NGC_3077.
- NGC_3077 sameAs NGC_3077.
- NGC_3077 sameAs m.0b4m5x.
- NGC_3077 sameAs Q744997.
- NGC_3077 sameAs Q744997.
- NGC_3077 wasDerivedFrom NGC_3077?oldid=539756158.
- NGC_3077 depiction NGC_3077_Hubble.jpg.
- NGC_3077 isPrimaryTopicOf NGC_3077.
- NGC_3077 name "NGC 3077".
- NGC_3077 name "UGC 5398, PGC 29146".
