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NGC 5260

NGC 5260
The barred spiral galaxy NGC 5260
Observation data (J2000 epoch)
ConstellationHydra
Right ascension13h 40m 19.8871s[1]
Declination−23° 51′ 28.813″[1]
Redshift0.021688[1]
Heliocentric radial velocity6502 ± 7 km/s[1]
Distance326.6 ± 22.9 Mly (100.13 ± 7.02 Mpc)[1]
Group or clusterRR 254
Apparent magnitude (V)12.8[1]
Characteristics
TypeSB(s)c[1]
Size~248,900 ly (76.32 kpc) (estimated)[1]
Apparent size (V)1.6′ × 1.4′[1]
Other designations
IRAS 13375-2336, 2MASX J13401990-2351291, MCG -04-32-050, PGC 48371, ESO 509- G 092, RR 254a[1]

NGC 5260 is a barred spiral galaxy in the constellation of Hydra. Its velocity with respect to the cosmic microwave background is 6789 ± 21 km/s, which corresponds to a Hubble distance of 100.13 ± 7.02 Mpc (∼327 million light-years).[1] It was discovered by American astronomer Lewis Swift on 6 April 1885.[2]

According to the SIMBAD database, NGC 5260 is a Seyfert II galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[3]

NGC 5260 forms a physical pair with galaxy ESO 509- G 093, collectively named RR 254, with an optical separation of 241″ between them.[4]

Supernovae

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Two supernovae have been observed in NGC 5260:

See also

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References

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  1. ^ a b c d e f g h i j k "Results for object NGC 5260". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 9 August 2024.
  2. ^ Seligman, Courtney. "Celestial Atlas Entry for NGC 5260". cseligman.com. Retrieved 9 August 2024.
  3. ^ "NGC 5260". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 December 2024.
  4. ^ Reduzzi, L; Rampazzo, R. (1995). "Candidates for a southern extension of the Karachentsev catalogue of isolated pairs of galaxies". Astrophysical Letters and Communications. 30: 1–229. Bibcode:1995ApL&C..30....1R.
  5. ^ "SN 2022jkx". Transient Name Server. IAU. Retrieved 16 December 2024.
  6. ^ "SN 2023dtd". Transient Name Server. IAU. Retrieved 16 December 2024.
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