NGC 3689 is an intermediate spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 3049 ± 22 km/s, which corresponds to a Hubble distance of 44.97 ± 3.16 Mpc (∼147 million light-years).[1] However, 16 non-redshift measurements give a distance of 39.350 ± 2.088 Mpc (∼128 million light-years).[1] The galaxy was discovered by German-British astronomer William Herschel on 6 April 1785.[2]

NGC 3689
The intermediate spiral galaxy NGC 3689.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 28m 11.0268s[1]
Declination+25° 39′ 40.22″[1]
Redshift0.009130 [1]
Heliocentric radial velocity2737 ± 1 km/s[1]
Distance146.7 ± 10.3 Mly (44.97 ± 3.16 Mpc)[1]
Apparent magnitude (V)12.3[1]
Characteristics
TypeSAB(rs)c[1]
Size~69,100 ly (21.20 kpc) (estimated)[1]
Apparent size (V)1.7' x 1.1'[1]
Other designations
2MASX J11281100+2539397, UGC 6467, MCG +04-27-037, PGC 35294, CGCG 126-057[1]

According to the SIMBAD database, NGC 3689 is a radio galaxy.[3]

The SAGA Astronomical Survey for the search for satellite galaxies orbiting another galaxy confirmed the presence of two satellite galaxies for NGC 3689.[4]

One calcium-rich supernova has been observed in NGC 3689: AT 2024mxe (type Gap, mag. 17.7).[5]

See also

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References

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  1. ^ a b c d e f g h i j k l "NASA/IPAC Extragalactic Database". Results for NGC 3689. Retrieved 8 August 2024.
  2. ^ Seligman, Courtney. "Celestial Atlas Entry for NGC 3689". cseligman.com. Retrieved 8 August 2024.
  3. ^ "SIMBAD astronomical database". Entry for NGC 3689. Retrieved 8 August 2024.
  4. ^ Mao, Yao-Yuan; Geha, Marla; Wechsler, Risa H.; Weiner, Benjamin; Tollerud, Erik J.; Nadler, Ethan O.; Kallivayalil, Nitya (2021). "The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way–like Galaxies". The Astrophysical Journal. 907 (2): 85. arXiv:2008.12783. Bibcode:2021ApJ...907...85M. doi:10.3847/1538-4357/abce58.
  5. ^ "Transient Name Server". Entry for AT 2024mxe. Retrieved 8 August 2024.
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