NGC 5548

radio jet[8] | |
---|---|
Other designations | |
Mrk 1509, UGC 9149[8] |
NGC 5548 is a Type I
In 1943, this galaxy was one of twelve
Among astronomers, the accepted explanation for the active nucleus in NGC 5548 is the accretion of matter onto a supermassive black hole (SMBH) at the core. This object is surrounded by an orbiting disk of accreted matter drawn in from the surroundings. As material is drawn into the outer parts of this disk, it becomes photoionized, producing broad emission lines in the optical and ultraviolet bands of the electromagnetic spectrum. A wind of ionized matter, organized in filamentary structures at distances of 1–14 light days from the center, is flowing outward in the direction perpendicular to the accretion disk plane.[9]
The mass of the central black hole can be estimated based on the properties of the emission lines in the core region. Combined measurements yield an estimated mass of 6.54+0.26
−0.25×107
References
- ^ "Swiftly moving gas streamer eclipses supermassive black hole". ESA/Hubble Press Release. Retrieved 20 June 2014.
- ^ S2CID 18913331.
- Bibcode:2009yCat.2294....0A.
- ^ S2CID 14911447. See footnote 2.
- ^ S2CID 11672751.
- ^ doi:10.1086/110721.
- ^ S2CID 119263271. See Table 1.
- ^ a b "NED results for object NGC 5548", NASA/IPAC Extragalactic Database, retrieved 2013-05-27.
- ^ S2CID 119117740.
- ^ S2CID 14081378.
- doi:10.1086/144488. See footnote 2.
- doi:10.1086/147580.
- doi:10.1071/ph660565.
- Bibcode:1968SvA....11..553D.
- S2CID 62879296.
- S2CID 7671684.
External links
- NGC 5548 on
- "NGC 5548: Chandra Reads the Cosmic Bar Code of Gas Around a Giant Black Hole", Chandra X-ray Observatory, Harvard-Smithsonian Center for Astrophysics, February 20, 2009, retrieved 2013-05-27.
- "Seyfert Galaxy NGC 5548 versus normal galaxy NGC 3277", UA astronomical image gallery, The University of Alabama, July 1999, retrieved 2013-05-27.