NGC 3783

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NGC 3783
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Artist's impression of the surroundings of the supermassive black hole in NGC 3783
Observation data
Constellation Centaurus
Right ascension 11h 39m 01.721s[1]
Declination –37° 44′ 18.60″[1]
Redshift 0.008506 ± 0.000100[2]
Helio radial velocity +2,817[3] km/s
Distance 135.7 e6ly (41.60[4] Mpc)
Group or cluster NGC 3783 group
Type SBa[5]
Apparent dimensions (V) 1′.9 × 1′.7[5]
Apparent magnitude (V) 13.43
Notable features Seyfert 1
See also: Galaxy, List of galaxies
This video shows an artist’s impression of the dusty wind emanating from the black hole at the centre of galaxy NGC 3783

NGC 3783 is a barred spiral galaxy located about 30[4] million light years away in the constellation Centaurus.[6] It is inclined by an angle of 23° to the line of sight from the Earth along a position angle of about 163°. The morphological classification of SBa[5] indicates a bar structure across the center (B) and tightly-wound spiral arms (a).[7] Although not shown by this classification, observers note the galaxy has a luminous inner ring surrounding the bar structure. The bright compact nucleus is active and categorized as a Seyfert 1 type. This nucleus is a strong source of X-ray emission and undergoes variations in emission across the electromagnetic spectrum.[5]

The source of the activity in this galaxy is a rapidly rotating supermassive black hole, which is located at the core and is surrounded by an accretion disk of dust.[8] The estimated mass of this black hole is 8.7 million ([8.7 ± 1.1] × 106) times the mass of the Sun.[9] Interferometric observations yield an inner radius of 0.52 ± 0.16 ly (0.16 ± 0.05 pc) for the orbiting torus of dust.[10]

This is a member of a loose association of 47 galaxies known as the NGC 3783 group. Located at a mean distance of 117 million light-years (36 Mpc), the group is centered at coordinates α = 11h 37m 12s, δ = –37° 30′ 57.6″: equivalent to about 870×10^3 ly (267 kpc) from NGC 3783. The NGC 3783 group has a mean velocity of 2,903 ± 26 km/s with respect to the Sun and a velocity dispersion of 190 ± 24 km/s. The diffuse X-ray emission of the group is roughly centered on the galaxy NGC 3783.[11]

References

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External links

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Coordinates: Sky map 11h 39m 01.721s, −-37° 44′ 18.60″