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- 3C_75 abstract "3C75 (aka 3C 75) is a binary black hole system in the Abell 400 cluster of galaxies. It has four radio jets (two from each accreting black hole). It is travelling at 1200 kilometers per second through the cluster plasma, causing the jets to be swept back. The binary supermassive black holes are themselves contained in the dumbbell shaped galaxy NGC 1128. 3C 75 may be X-ray source 2A 0252+060 (1H 0253+058, XRS 02522+060).".
- 3C_75 thumbnail 3c75.jpg?width=300.
- 3C_75 wikiPageExternalLink AladinPreview?02%2057%2041.7%20%2B06%2001%2028&ident=MCG%2B01-08-027.
- 3C_75 wikiPageExternalLink ap100314.html.
- 3C_75 wikiPageExternalLink lrr-2005-8.
- 3C_75 wikiPageExternalLink sim-id.pl?protocol=html&Ident=3C75.
- 3C_75 wikiPageExternalLink sim-id.pl?protocol=html&Ident=3c75&NbIdent=1&Radius=10&Radius.unit=arcmin&CooFrame=FK5&CooEpoch=2000&CooEqui=2000&output.max=all&o.catall=on&output.mesdisp=N&Bibyear1=1983&Bibyear2=2006&Frame1=FK5&Frame2=FK4&Frame3=G&Equi1=2000.0&Equi2=1950.0&Equi3=2000.0&Epoch1=2000.0&Epoch2=1950.0&Epoch3=2000.0.
- 3C_75 wikiPageExternalLink sim-id?protocol=html&Ident=MCG%2B01-08-027&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id.
- 3C_75 wikiPageExternalLink level3.php?id=30.
- 3C_75 wikiPageID "4716700".
- 3C_75 wikiPageRevisionID "589766081".
- 3C_75 appmagV "+13.93".
- 3C_75 constellationName Cetus.
- 3C_75 distLy "296".
- 3C_75 epoch Epoch_(astronomy).
- 3C_75 hasPhotoCollection 3C_75.
- 3C_75 name "Active Galaxy pair 3C75".
- 3C_75 names "MCG+01-08-027, NGC 1128".
- 3C_75 notes "contains binary black hole".
- 3C_75 sizeV "0.741".
- 3C_75 type "Active binary".
- 3C_75 z "0.0231".
- 3C_75 subject Category:3C_objects.
- 3C_75 subject Category:Abell_400.
- 3C_75 subject Category:Cetus_(constellation).
- 3C_75 subject Category:Radio_galaxies.
- 3C_75 subject Category:Supermassive_black_holes.
- 3C_75 type CelestialBody.
- 3C_75 type Galaxy.
- 3C_75 type PhysicalBody.
- 3C_75 comment "3C75 (aka 3C 75) is a binary black hole system in the Abell 400 cluster of galaxies. It has four radio jets (two from each accreting black hole). It is travelling at 1200 kilometers per second through the cluster plasma, causing the jets to be swept back. The binary supermassive black holes are themselves contained in the dumbbell shaped galaxy NGC 1128. 3C 75 may be X-ray source 2A 0252+060 (1H 0253+058, XRS 02522+060).".
- 3C_75 label "3C 75".
- 3C_75 label "3C 75".
- 3C_75 label "3C 75".
- 3C_75 sameAs 3C_75.
- 3C_75 sameAs 3C_75.
- 3C_75 sameAs m.0cjtz6.
- 3C_75 sameAs Q3315001.
- 3C_75 sameAs Q3315001.
- 3C_75 wasDerivedFrom 3C_75?oldid=589766081.
- 3C_75 depiction 3c75.jpg.
- 3C_75 isPrimaryTopicOf 3C_75.
- 3C_75 name "Active Galaxy pair 3C75".
- 3C_75 name "MCG+01-08-027, NGC 1128".
