NGC 7793

NGC 7793
Hubble Space Telescope image of the small bulge and spiral arms of NGC 7793
Observation data (J2000 epoch)
ConstellationSculptor
Right ascension23h 57m 49.753s[1]
Declination−32° 35′ 27.71″[1]
Heliocentric radial velocity227 km/s[2]
Distance12.2 Mly (3.7 Mpc)[3]
Group or clusterSculptor Group[4]
Apparent magnitude (V)10.0[5]
Characteristics
TypeSA(s)d[6]
MassStellar: 3.2×109 M☉
Apparent size (V)9.3′ × 6.3′[5] (~30kly in diameter)
Other designations
NGC 7793, PGC 73049[7]
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NGC 7793 is a flocculent spiral galaxy in the southern constellation of Sculptor. It was discovered in 1826 by Scottish astronomer James Dunlop.[8] The galaxy is located at a distance of 12.2[3] million light years and is receding with a heliocentric radial velocity of 227 km/s.[2] NGC 7793 is one of the five brightest galaxies within the Sculptor Group.[5][4]

The morphological class of NGC 7793 is SA(s)d,[6] indicating it is unbarred spiral galaxy (SA) with no inner ring structure (s) and the arms are loosely wound and disorganized (d). It is flocculent in appearance with a very small bulge and a star cluster at the nucleus.[5] The galactic disk is inclined at an angle of 53.7° to the line of sight from the Earth. The visible profile is elliptical in form with an angular size of 9.3′ × 6.3′[5] and a major axis aligned along a position angle of 99.3°.[6] There are two nearby dwarf galaxy companions.[9]

On March 25, 2008, a type II-P supernova designated SN 2008bk was discovered in NGC 7793.[10][6] At apparent magnitude 12.5, it became the 2nd brightest supernova of 2008.[11] The progenitor of this supernova was a red supergiant, observed only 547 days prior to the explosion.

Jets from a black hole named P13 power a large nebula designated S26 in the outer spiral of this galaxy. Recently, the mass of P13 was determined to be less than 15 solar masses, and its companion star is estimated to be around 20 solar masses. The two orbit each other in 64 days.[12] Based on this estimate, P13 is stripping material away from a nearby star about ten times faster than was previously believed to be physically possible. If correct, this observation would show flaws in theories that a black hole's mass and rate of consumption are a fixed relationship.[13][14]

  1. ^ a b Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  2. ^ a b Cite error: The named reference Tully_et_al_2016 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference Lianou_et_al_2019 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference karachentsevetal2003 was invoked but never defined (see the help page).
  5. ^ a b c d e Cite error: The named reference König_Binnewies_2017 was invoked but never defined (see the help page).
  6. ^ a b c d Cite error: The named reference Crowther2013 was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference ned was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference Dunlop1828 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference Mondal_et_al_2021 was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference SN2008bk was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference supernovae2008 was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference icrar was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference io9 was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference ifls was invoked but never defined (see the help page).