NGC 6794

Galaxy in the constellation Sagittarius From Wikipedia, the free encyclopedia

NGC 6794 is a large spiral galaxy in the constellation of Sagittarius. Its velocity with respect to the cosmic microwave background is 5,887±13 km/s, which corresponds to a Hubble distance of 283.2 ± 19.8 Mly (86.83 ± 6.08 Mpc).[1] However, three non-redshift measurements give a farther mean distance of 315.94 ± 1.96 Mly (96.867 ± 0.601 Mpc).[2] It was discovered by British astronomer John Herschel on 24 August 1834.[3][4]

Right ascension19h 28m 03.8849s[1]
Declination−38° 55 07.297[1]
Redshift0.020077±0.0000300[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 6794
NGC 6794 imaged by Legacy Surveys
Observation data (J2000 epoch)
ConstellationSagittarius
Right ascension19h 28m 03.8849s[1]
Declination−38° 55 07.297[1]
Redshift0.020077±0.0000300[1]
Heliocentric radial velocity6,019±9 km/s[1]
Distance315.94 ± 1.96 Mly (96.867 ± 0.601 Mpc)[1]
Group or clusterLDC 1344
Apparent magnitude (V)13.9[1]
Characteristics
TypeSA(rs)ab[1]
Size~229,700 ly (70.44 kpc) (estimated)[1]
Apparent size (V)1.7′ × 1.5′[1]
Other designations
ESO 338- G 005, 2MASX J19280388-3855077, MCG -07-40-001, PGC 63241[1]
Close

NGC 6794 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[5][6]

NGC 6794 viewed through visible light

Galaxy group

NGC 6794 is a member of a small galaxy group known as LDC 1344, which includes the galaxies ESO 338-7 [d] and ESO 338-9 [d].[7][8]

Supernova

One supernova has been observed in NGC 6794:

  • SN 2024dgn (Type Ia, mag. 15.719) was discovered by ATLAS on 26 February 2024.[9]

See also

References

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