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NGC 6106
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NGC 6106
NGC 6106 imaged by SDSS
Observation data (J2000 epoch)
ConstellationHercules
Right ascension16h 18m 47.1712s[1]
Declination+07° 24′ 39.319″[1]
Redshift0.004833±0.000002[1]
Heliocentric radial velocity1,449±1 km/s[1]
Distance72.64 ± 2.49 Mly (22.272 ± 0.764 Mpc)[1]
Apparent magnitude (V)12.84[1]
Characteristics
TypeSA(s)c[1]
Size~55,600 ly (17.04 kpc) (estimated)[1]
Apparent size (V)2.5′ × 1.4′[1]
Other designations
IRAS 16163+0731, 2MASX J16184720+0724396, UGC 10328, MCG +01-41-016, PGC 57799, CGCG 052-001[1]

NGC 6106 is a spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 1,527±6 km/s, which corresponds to a Hubble distance of 73.5 ± 5.2 Mly (22.52 ± 1.58 Mpc).[1] This is in good agreement with 29 non-redshift measurements which give an average distance of 72.64 ± 2.49 Mly (22.272 ± 0.764 Mpc).[2] It was discovered by German-British astronomer William Herschel on 13 April 1784.[3][4]

Luminous red nova and supernova

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One luminous red nova and one supernova have been observed in NGC 6106:

  • AT 2020kog (type LRN, mag. 20.3) was discovered by Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) Search for Kilonovae on 18 May 2020.[5][6]
  • SN 2024ahv (Type Ib, mag. 16.2) was discovered by Japanese astronomer Hidehiko Okoshi on 16 January 2024.[7]

See also

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References

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