Arp 166: Difference between revisions
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{{short description|Interacting galaxy pair}} |
{{short description|Interacting galaxy pair}} |
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{{Infobox Galaxy |
{{Infobox Galaxy |
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| name = |
| name = felix piss off]] 166 |
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| image = NGC750 - NGC751 - SDSS DR14.png |
| image = NGC750 - NGC751 - SDSS DR14.png |
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| caption = Arp 166 consists of [[NGC 750]] (top) and [[NGC 751]] (bottom) ([[Sloan Digital Sky Survey|SDSS]]) |
| caption = Arp 166 consists of [[NGC 750]] (top) and [[NGC 751]] (bottom) ([[Sloan Digital Sky Survey|SDSS]]) |
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Revision as of 03:00, 19 January 2021
| felix piss off]] 166 | |
|---|---|
 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Triangulum |
| Right ascension | 01h 57m 32.00s [1] |
| Declination | +33° 12′ 24.00″ [1] |
| Redshift | 0.017529 [2] |
| Heliocentric radial velocity | 5255 km/s [2] |
| Distance | 225 Mly [3] |
| Apparent magnitude (B) | 12.90 [1] |
| Characteristics | |
| Type | Pair of galaxies E0+E [2] |
| Apparent size (V) | 2.5 x 1.7 [2] |
| Other designations | |
| NGC 750, NGC 751 | |
Arp 166 is a pair of interacting elliptical galaxies approximately 225 million light-years away from Earth in the constellation of Triangulum.[2][3] The two galaxies, NGC 750 and NGC 751, are listed together as Arp 166 in the Atlas of Peculiar Galaxies (in the category Galaxies with diffuse filaments).[4]
Observational history
Arp 166 was discovered by German-born British astronomer William Herschel on September 12, 1784, but he did not resolve this close pair of galaxies, therefore he described it as a single object NGC 750.[4][3]
Arp 166 was first seen as a double by Irish engineer and astronomer Bindon Stoney on October 11, 1850, who used Lord Rosse's 72" telescope.[4] The second galaxy from this pair, which is smaller and fainter than NGC 750, was catalogued as NGC 751.[4]
Interacting galaxies
At least 100,000,000 years have passed since the moment of the first strong tidal perturbation between these two galaxies.[5] Both galaxies are characterized by strong tidal interactions and distortions, and they are still in the process of efficient tidal interaction.[5]
The distance between the centers of this pair is 21", or 10 kpc in projection.[6][5] Both galaxies have almost identical central radial velocities.[5] While NGC 750 exhibits nearly flat radial velocity curves, the radial velocity curves of NGC 751 are characterized by large variations of more than 100 km s−1 along the slit.[5]
A large, diffuse tidal tail extends 20 arcsec (10 kpc) to the north-east of the pair.[5]
See also
References
- ^ a b c "SIMBAD Astronomical Database". Retrieved March 7, 2019.
- ^ a b c d e "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved March 7, 2019.
- ^ a b c "Focal Pointe Observatory". bf-astro.com. Retrieved March 7, 2019.
- ^ a b c d "Data for NGC 750/751". www.astronomy-mall.com. Retrieved March 7, 2019.
- ^ a b c d e f Madejsky, R. (1991). "Morphology and kinematics of the interacting elliptical galaxies NGC750 and NGC751 = ARP 166 - Velocity fields of tidally distorted elliptical galaxies". Astronomy and Astrophysics. 247: 348–356. Bibcode:1991A&A...247..348M.
- ^ Sandage, A.; Bedke, J. (1994). The Carnegie Atlas of Galaxies. Volume I. Carnegie Institution of Washington. Bibcode:1994cag..book.....S.
External links
- Arp 166 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images