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- NGC_5090_and_NGC_5091 abstract "NGC 5090 and NGC 5091 are a set of galaxies approximately 150 million light-years away in the constellation Centaurus. They are in the process of colliding and merging with some evidence of tidal disruption of NGC 5091. NGC 5090 is an elliptical galaxy while NGC 5091 is a spiral galaxy. The velocity of the nucleus of NGC 5091 has been measured as 3429 km/s, while NGC 5090 has a velocity of 3185 km/s. NGC 5090 is associated with a strong, double radio source (PKS 1318-43).".
- NGC_5090_and_NGC_5091 thumbnail Phot-20d-99-hires.jpg?width=300.
- NGC_5090_and_NGC_5091 wikiPageExternalLink ap971205.html.
- NGC_5090_and_NGC_5091 wikiPageExternalLink phot-20-99.html.
- NGC_5090_and_NGC_5091 wikiPageID "4737856".
- NGC_5090_and_NGC_5091 wikiPageRevisionID "544347307".
- NGC_5090_and_NGC_5091 appmagV "12.6".
- NGC_5090_and_NGC_5091 caption "NGC 5090/5091".
- NGC_5090_and_NGC_5091 constellationName Centaurus.
- NGC_5090_and_NGC_5091 dec "/".
- NGC_5090_and_NGC_5091 distLy "150".
- NGC_5090_and_NGC_5091 epoch Epoch_(astronomy).
- NGC_5090_and_NGC_5091 hasPhotoCollection NGC_5090_and_NGC_5091.
- NGC_5090_and_NGC_5091 name "NGC 5090 and NGC 5091".
- NGC_5090_and_NGC_5091 names "PGC 46618 / 46626".
- NGC_5090_and_NGC_5091 notes Interacting_galaxy.
- NGC_5090_and_NGC_5091 ra "/".
- NGC_5090_and_NGC_5091 sizeV "2".
- NGC_5090_and_NGC_5091 type "E2 / Sb pec sp".
- NGC_5090_and_NGC_5091 z "3420".
- NGC_5090_and_NGC_5091 subject Category:Centaurus_(constellation).
- NGC_5090_and_NGC_5091 subject Category:Elliptical_galaxies.
- NGC_5090_and_NGC_5091 subject Category:Interacting_galaxies.
- NGC_5090_and_NGC_5091 subject Category:NGC_objects.
- NGC_5090_and_NGC_5091 subject Category:PGC_objects.
- NGC_5090_and_NGC_5091 subject Category:Peculiar_galaxies.
- NGC_5090_and_NGC_5091 subject Category:Spiral_galaxies.
- NGC_5090_and_NGC_5091 type CelestialBody.
- NGC_5090_and_NGC_5091 type Galaxy.
- NGC_5090_and_NGC_5091 type PhysicalBody.
- NGC_5090_and_NGC_5091 comment "NGC 5090 and NGC 5091 are a set of galaxies approximately 150 million light-years away in the constellation Centaurus. They are in the process of colliding and merging with some evidence of tidal disruption of NGC 5091. NGC 5090 is an elliptical galaxy while NGC 5091 is a spiral galaxy. The velocity of the nucleus of NGC 5091 has been measured as 3429 km/s, while NGC 5090 has a velocity of 3185 km/s. NGC 5090 is associated with a strong, double radio source (PKS 1318-43).".
- NGC_5090_and_NGC_5091 label "NGC 5090 and NGC 5091".
- NGC_5090_and_NGC_5091 sameAs m.0ckqfh.
- NGC_5090_and_NGC_5091 sameAs Q3341278.
- NGC_5090_and_NGC_5091 sameAs Q3341278.
- NGC_5090_and_NGC_5091 wasDerivedFrom NGC_5090_and_NGC_5091?oldid=544347307.
- NGC_5090_and_NGC_5091 depiction Phot-20d-99-hires.jpg.
- NGC_5090_and_NGC_5091 isPrimaryTopicOf NGC_5090_and_NGC_5091.
- NGC_5090_and_NGC_5091 name "NGC 5090 and NGC 5091".
- NGC_5090_and_NGC_5091 name "PGC 46618 / 46626".