Summary
NGC 6810 is a spiral galaxy approximately 87 million light-years away from Earth in the constellation of Pavo.[1]
| NGC 6810 | |
|---|---|
 NGC 6810 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Pavo |
| Right ascension | 19h 43m 34.25s [1] |
| Declination | −58° 39′ 20.12″ [1] |
| Redshift | 0.006775 [1] |
| Heliocentric radial velocity | 2031 ± 10 km/s [1] |
| Distance | 87 Mly[1] |
| Apparent magnitude (V) | 11.60 [2] |
| Apparent magnitude (B) | 12.40 [2] |
| Characteristics | |
| Type | SA(s)ab:sp [1] |
| Apparent size (V) | 3.2 x 0.9 [1] |
| Other designations | |
| PGC 63571, ESO 142-35 | |
Observational history edit
NGC 6810 was discovered by John Herschel on July 10, 1834.[3] It was later added to the New General Catalogue by John Louis Emil Dreyer.
Misclassification of NGC 6810 edit
This galaxy used to be classified as a Seyfert 2 galaxy, but that is probably incorrect.[4] Recent X-ray observations provide no evidence of any active galactic nucleus (AGN) activity,[4] and high resolution optical spectra do not confirm the status of NGC 6810 as a Seyfert galaxy, thus it appears to have been misclassified.[4][5]
Features edit
NGC 6810 is an early-type spiral of roughly equivalent mass to the Milky Way.[4] X-ray, optical, IR and radio properties of NGC 6810 are all consistent with a starburst galaxy.[4]
Galactic-scale superwind edit
Observation of NGC 6810 with XMM-Newton reveals the presence of extended soft X-ray emission within the optical disc of the galaxy (which is closely associated with star-forming regions) and also beyond the optical disc.[4] This, along with Hα filamentation and peculiar minor axis ionized gas kinematics, strongly suggest that NGC 6810 is host to a galactic-scale superwind[4] which is streaming from the starburst region.[6]
The actively star-forming regions and the base radius of the outflow are unusually spread out, and extend out to a radius of ~6.5 kpc from the nucleus. Most superwinds in other galaxies appear to arise in ≲ 1 kpc-scale nuclear starburst regions.[4] That makes NGC 6810 one of the few ‘disc-wide’ superwinds currently known,[4] because NGC 6810's superwind base extends across nearly 70 percent of the entire galaxy's diameter.[6] Only three other starburst galaxies are known to have broad superwind sources.[6]
See also edit
References edit
- ^ a b c d e f g h "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 28 November 2017.
- ^ a b "Revised NGC Data for NGC 6810". spider.seds.org. Retrieved December 9, 2017.
- ^ "Data for NGC 6810". www.astronomy-mall.com. Retrieved December 9, 2017.
- ^ a b c d e f g h i Strickland, David K. (2007). "A new superwind galaxy: XMM–Newton observations of NGC 6810". Monthly Notices of the Royal Astronomical Society. 376 (2): 523–533. arXiv:astro-ph/0701630. Bibcode:2007MNRAS.376..523S. doi:10.1111/j.1365-2966.2007.11478.x. S2CID 13834527.
- ^ Forbes, Duncan A.; Norris, R. P. (1998). "Star Formation in Southern Seyfert Galaxies". Monthly Notices of the Royal Astronomical Society. 300 (3): 757. arXiv:astro-ph/9804298. Bibcode:1998MNRAS.300..757F. doi:10.1046/j.1365-8711.1998.01940.x. S2CID 3719096. Retrieved 3 December 2017.
- ^ a b c "Blowin' in the galactic superwind". www.astronomy.com. Retrieved 3 December 2017.
External links edit
- NGC 6810 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS