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- Q1106429 subject Q1031119.
- Q1106429 subject Q10641.
- Q1106429 subject Q7282683.
- Q1106429 subject Q8266666.
- Q1106429 abstract "NGC 3783 is a barred spiral galaxy located about 30 million light years away in the constellation Centaurus. 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 indicates a bar structure across the center (B) and tightly-wound spiral arms (a). 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.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. The estimated mass of this black hole is 8.7 million ([8.7 ± 1.1] × 106) times the mass of the Sun. Interferometric observations yield an inner radius of 0.52 ± 0.16 ly (0.16 ± 0.05 pc) for the orbiting torus of dust.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.".
- Q1106429 thumbnail Artists_impression_of_the_surroundings_of_the_supermassive_black_hole_in_NGC_3783.jpg?width=300.
- Q1106429 wikiPageExternalLink press_052500.html.
- Q1106429 wikiPageExternalLink eso1327.
- Q1106429 wikiPageWikiLink Q1031119.
- Q1106429 wikiPageWikiLink Q10641.
- Q1106429 wikiPageWikiLink Q12129.
- Q1106429 wikiPageWikiLink Q12510.
- Q1106429 wikiPageWikiLink Q1648748.
- Q1106429 wikiPageWikiLink Q17512228.
- Q1106429 wikiPageWikiLink Q180892.
- Q1106429 wikiPageWikiLink Q182429.
- Q1106429 wikiPageWikiLink Q2.
- Q1106429 wikiPageWikiLink Q2105737.
- Q1106429 wikiPageWikiLink Q213930.
- Q1106429 wikiPageWikiLink Q237604.
- Q1106429 wikiPageWikiLink Q2490.
- Q1106429 wikiPageWikiLink Q40392.
- Q1106429 wikiPageWikiLink Q46587.
- Q1106429 wikiPageWikiLink Q525.
- Q1106429 wikiPageWikiLink Q531.
- Q1106429 wikiPageWikiLink Q605931.
- Q1106429 wikiPageWikiLink Q7282683.
- Q1106429 wikiPageWikiLink Q8266666.
- Q1106429 wikiPageWikiLink Q850283.
- Q1106429 wikiPageWikiLink Q8844.
- Q1106429 wikiPageWikiLink Q8928.
- Q1106429 name "NGC 3783".
- Q1106429 type Place.
- Q1106429 type CelestialBody.
- Q1106429 type Galaxy.
- Q1106429 type Location.
- Q1106429 type Place.
- Q1106429 type Thing.
- Q1106429 type Q318.
- Q1106429 comment "NGC 3783 is a barred spiral galaxy located about 30 million light years away in the constellation Centaurus. 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 indicates a bar structure across the center (B) and tightly-wound spiral arms (a). Although not shown by this classification, observers note the galaxy has a luminous inner ring surrounding the bar structure.".
- Q1106429 label "NGC 3783".
- Q1106429 depiction Artists_impression_of_the_surroundings_of_the_supermassive_black_hole_in_NGC_3783.jpg.
- Q1106429 name "NGC 3783".