NGC 2340

Galaxy in the constellation Lynx From Wikipedia, the free encyclopedia

NGC 2340 is a large elliptical galaxy in the constellation of Lynx. Its velocity with respect to the cosmic microwave background is 6,008±9 km/s, which corresponds to a Hubble distance of 289.0 ± 20.3 Mly (88.61 ± 6.21 Mpc).[1] However, six non-redshift measurements give a farther mean distance of 315.77 ± 44.34 Mly (96.817 ± 13.596 Mpc).[2] It was discovered by German-British astronomer William Herschel on 9 February 1788.[3]

Right ascension07h 11m 10.7950s[1]
Declination+50° 10 29.075[1]
Redshift0.019764±0.0000250[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 2340
NGC 2340 imaged by Pan-STARRS
Observation data (J2000 epoch)
ConstellationLynx
Right ascension07h 11m 10.7950s[1]
Declination+50° 10 29.075[1]
Redshift0.019764±0.0000250[1]
Heliocentric radial velocity5,925±7 km/s[1]
Distance315.77 ± 44.34 Mly (96.817 ± 13.596 Mpc)[1]
Apparent magnitude (V)12.7[1]
Characteristics
TypeE[1]
Size~263,000 ly (80.64 kpc) (estimated)[1]
Apparent size (V)1.8′ × 1.2′[1]
Other designations
2MASX J07111080+5010288, UGC 3720, MCG +08-13-096, PGC 20338, CGCG 234-091[1]
Close

NGC 2340 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[4][5]

Abell 569 member

NGC 2340 is a member of the Abell 569 galaxy cluster, which contains 85 galaxies, the brightest of which is NGC 2329 [fr].[6]

Supernova

One supernova has been observed in NGC 2340:

See also

References

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