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NGC 4260

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NGC 4260
NGC 4260 imaged by the Vera C. Rubin Observatory
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 19m 22.2554s[1]
Declination+06° 05′ 55.482″[1]
Redshift0.006531[1]
Heliocentric radial velocity1,776±2 km/s[1]
Distance131.33 ± 6.17 Mly (40.267 ± 1.891 Mpc)[1]
Apparent magnitude (B)13.1[2]
Characteristics
TypeSB(s)a[1]
Size~142,600 ly (43.73 kpc) (estimated)[1]
Apparent size (V)3.34′ × 1.03′[1]
Other designations
UGC 7361, MCG +01-31-054, PGC 39656, CGCG 042-015[2][1]

NGC 4260 is a barred spiral galaxy in the constellation Virgo. Its velocity with respect to the cosmic microwave background is 2,122±24 km/s, which corresponds to a Hubble distance of 102.1 ± 7.2 Mly (31.29 ± 2.22 Mpc).[1] However, six non-redshift measurements give a much farther distance of 131.33 ± 6.17 Mly (40.267 ± 1.891 Mpc).[3] It was discovered by German-British astronomer William Herschel on 13 April 1784.[4][5]

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See also

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References

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  1. ^ a b c d e f g h i j "Results for object NGC 4260". NASA/IPAC Extragalactic Database. Retrieved 3 May 2019.
  2. ^ a b "NGC 4260". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 3 May 2019.
  3. ^ "Distance Results for NGC 4260". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 5 July 2025.
  4. ^ Herschel, W. (1786). "Catalogue of One Thousand New Nebulae and Clusters of Stars" (PDF). Philosophical Transactions of the Royal Society of London. 76: 457–499. Bibcode:1786RSPT...76..457H. doi:10.1098/rstl.1786.0027.
  5. ^ Seligman, Courtney. "New General Catalog Objects: NGC 4250 - 4299". cseligman.com. Retrieved 3 May 2019.
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