NGC 4800
2MASX J12543777+4631521[4] |
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NGC 4800 is an isolatedspiral arms (b). The galactic plane is inclined to the line of sight by an angle of 43°, and the long axis is oriented along a position angle of 25°.[8] There is a weak bar structure at the nucleus that is visible in the infrared.[6]
The galaxy has a low-luminosity
HII region at the core.[5] The circumnuclear zone contains a double ring structure of "ultra-compact nuclear rings"; the inner ring has a radius of 30 pc and the outer ring's radius is about 130 pc.[6] The upper limit on the mass of the central supermassive black hole is estimated as 2.0×107 M☉, or 20 million times the mass of the Sun.[9]
References
- ^ .
- ^ a b "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 31 May 2019.
- ^ .
- ^ a b "NGC 4800". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 31 May 2019.
- ^ S2CID 119471662.
- ^ S2CID 14678950.
- ^ Seligman, Courtney. "New General Catalog Objects: NGC 4800 - 4849". New General Catalog Objects: NGC 4800 - 4849. Retrieved 31 May 2019.
- S2CID 17982236.
- S2CID 50115334.
External links
- Media related to NGC 4800 at Wikimedia Commons
- NGC 4800 on