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NGC 2935 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Hydra |
Right ascension | 09h 36m 44.8615s[1] |
Declination | −21° 07′ 41.53″[1] |
Redshift | 0.007575[1] |
Heliocentric radial velocity | 2271 ± 3 km/s[1] |
Distance | 90.97 ± 2.40 Mly (27.890 ± 0.736 Mpc)[1] |
Apparent magnitude (V) | 12.1[1] |
Surface brightness | 23.9 mag/arcsec^2 |
Characteristics | |
Type | (R')SAB(s)b[1] |
Size | ~185,200 ly (56.79 kpc) (estimated)[1] |
Apparent size (V) | 3.7′ × 2.8′[1] |
Other designations | |
ESO 565- G 023, IRAS 09344-2054, UGCA 169, MCG -03-25-011, PGC 27351[1] |
NGC 2935 is a large intermediate spiral galaxy located in the constellation Hydra. Its speed relative to the cosmic microwave background is 2,601 ± 23 km/s, which corresponds to a Hubble distance of 38.4 ± 2.7 Mpc (~125 million ly). It was discovered by German-British astronomer William Herschel on 20 March 1786.[1][2]
NGC 2935 was used by Gérard de Vaucouleurs as a galaxy of morphological type (R2')SAB(s)b in his galaxy atlas. The luminosity class of NGC 2935 is II and it has a broad HI line. In addition, it is a star-forming burst galaxy.[3]
To date, 29 studies and measurements based on redshift give a distance of 27.890 ± 3.962 Mpc (~91 million ly),[4] which is outside the Hubble distance values. Note that it is with the average value of independent measurements, when they exist, that the NASA/IPAC database calculates the diameter of a galaxy and that consequently the diameter of NGC 2935 could be approximately 78, 1 kpc (~255,000 ly) if we used the Hubble distance to calculate it.[5]
Observations from the Hubble Space Telescope have concluded that a star-forming disk is present around the core of NGC 2935. The size of its semi-major axis is estimated at 530 pc (~1730 light years) at the estimated distance of this galaxy.[6]
Four supernovae have been discovered in NGC 2935:
NGC 2935 is part of a small group of three galaxies named after it. The other two galaxies in the NGC 2935 group are NGC 2983 and NGC 2986.[13]