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NGC 1511

NGC 1511
The barred spiral galaxy NGC 1511.
Observation data (J2000 epoch)
ConstellationHydrus
Right ascension03h 59m 36.98s[1]
Declination−67° 38′ 03.3″[1]
Redshift0.004474[1]
Heliocentric radial velocity1341 ± 5 km/s[1]
Distance64.4 ± 4.5 Mly (19.76 ± 1.39 Mpc)[1]
Apparent magnitude (V)11.3[1]
Characteristics
TypeSAa pec: HII[1]
Size~83,000 ly (25.45 kpc) (estimated)[1]
Apparent size (V)3.5' x 1.3'[1]
Other designations
IRAS 03594-6746, 2MASX J03593698-6738033, MCG +00-12-072, PGC 14236, ESO 055- G 004[1]

NGC 1511 is a barred spiral galaxy in the constellation of Hydrus. Its velocity with respect to the cosmic microwave background is 1341 ± 5 km/s, which corresponds to a Hubble distance of 19.76 ± 1.39 Mpc (∼64 million light-years).[1] It was discovered by British astronomer John Herschel on 2 November 1834.

One supernova has been observed in NGC 1511: SN 1935C (type unknown, mag. 12.5).[2] The supernova was discovered by Emily Hughes Boyce on 16 August 1935, and was initially thought to be either a supernova, or a nova associated with the Large Magellanic Cloud. It was classified as a nova, and known as either HV 11970 or Nova Hydri 1935. In September 1988, Sidney Van Den Bergh and Martha L. Hazen concluded definitively that the object was a supernova in NGC 1511, and the star was given the designation SN 1935C.[3][4]

NGC 1511 Group

According to A.M. Garcia, the galaxy NGC 1511 is the central member of the NGC 1511 group (also known as LGG 107) that includes NGC 1473 and NGC 1511A .[5]

See also

References

  1. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 1511. Retrieved 28 July 2024.
  2. ^ Transient Name Server entry for SN 1935C. Retrieved 28 July 2024.
  3. ^ van den Bergh, Sidney; Hazen, Martha L. (1988). "Was Nova Hydri 1935 a Supernova?". Publications of the Astronomical Society of the Pacific. 100: 1542. Bibcode:1988PASP..100.1542V. doi:10.1086/132362.
  4. ^ Green, Daniel W. E. (August 25, 1988). "Central Bureau for Astronomical Telegrams, Circular No. 4647". Retrieved 21 August 2024.
  5. ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
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