NGC 4340 is a double-barred lenticular galaxy[2][3] located about 55 million light-years away[4] in the constellation of Coma Berenices.[5] NGC 4340 was discovered by astronomer William Herschel on March 21, 1784.[6] NGC 4340 is a member of the Virgo Cluster.[2][3] NGC 4340 is generally thought to be in a pair with the galaxy NGC 4350.[6][7]

NGC 4340
Hubble Space Telescope image of NGC 4340
Observation data (J2000 epoch)
Constellation	Coma Berenices
Right ascension	12h 23m 35.3s[1]
Declination	16° 43′ 20″[1]
Redshift	0.003112/933 km/s[1]
Distance	56,070,000 ly
Group or cluster	Virgo Cluster
Apparent magnitude (V)	12.10[1]
Characteristics
Type	SB0^+(r) [1]
Size	~ 53,400 ly
Apparent size (V)	3.5 x 2.8[1]
Other designations
CGCG 99-36, MCG 3-32-21, PGC 40245, UGC 7467, VCC 654[1]

Physical characteristics

NGC 4340 has a small inner bar embedded in a luminous stellar nuclear ring. Even though the ring is luminous, there are no star-forming regions. Instead, the ring is made of mostly old stars in a gas-poor environment. The color of the ring is the same as the color of the surrounding bulge suggesting that it is probably an old, “fossil” remnant of an earlier episode of star-formation.[2] Crossing the inner ring, there is a larger primary bar with ansae at the ends.[3] Careful inspection shows that the two bars are slightly misaligned, which suggests they may be independently rotating.[2] The larger primary bar connects to another ring that surrounds the central regions of the galaxy.[7]

SN1977A

On January 27, 1977 a supernova of an unknown type was discovered in NGC 4340.[8][9]

See also

• List of NGC objects (4001–5000)

References

External links

Wikimedia Commons has media related to NGC 4340.

• NGC 4340 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

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