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NGC 3535

From Wikipedia, the free encyclopedia
NGC 3535
The spiral galaxy NGC 3535.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 08m 33.92s[1]
Declination+04° 49′ 54.821″[1]
Redshift0.023103[1]
Heliocentric radial velocity6926 ± 2 km/s[1]
Distance350.7 ± 24.6 Mly (107.51 ± 7.54 Mpc)[1]
Apparent magnitude (V)13.5[1]
Characteristics
TypeSA(s)a pec?[1]
Size~162,300 ly (49.77 kpc) (estimated)[1]
Apparent size (V)1.7' x 0.8'[1]
Other designations
IRAS 11059+0505, 2MASX J11083390+0449545, UGC 6189, MCG +01-29-004, PGC 33760, CGCG 039-010[1]

NGC 3535 is a spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 7289 ± 25 km/s, which corresponds to a Hubble distance of 107.51 ± 7.54 Mpc (∼351 million light-years).[1] It was discovered by German-British astronomer William Herschel on 18 April 1784.

According to the SIMBAD database, NGC 3535 is a radio galaxy.[2]

One supernova has been observed in NGC 3535: SN 2023hrn (type Ia, mag. 18.4).[3]

See also

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References

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  1. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 3535. Retrieved 29 July 2024.
  2. ^ SIMBAD entry for NGC 3535. Retrieved 29 July 2024.
  3. ^ Transient Name Server entry for SN 2023hrn. Retrieved 29 July 2024.
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