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NGC 5940

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NGC 5940
Observation data (J2000 epoch)
ConstellationSerpens
Right ascension15h 31m 18.070s
Declination+07d 27m 27.91s
Redshift0.03405
Heliocentric radial velocity10,209 km/s
Distance500 Mly (153.3 Mpc)
Apparent magnitude (V)15.56
Characteristics
TypeSeyfert galaxy
Size140,000 ly
Other designations
PGC 55295, IRAS F15288+0737, UGC 9876, LEDA 55295, MRK 1511, MRK 9030, MCG +01-39-025

NGC 5940 is a barred spiral galaxy located in the Serpens constellation.[1][2][3] The galaxy was found on April 19, 1887, by Lewis Swift, an American astronomer.[2] NGC 5940 is located 500 million light-years away from the Milky Way and it is approximately 140,000 light-years across in diameter.[3][2]

NGC 5940 is a Seyfert type 1 galaxy and is considered a quasar according to the SIMBAD database.[4][5] It is registered under the Markarian Catalogue as Markarian 1511 or MRK 9030.[6] It has an bright active core, meaning there is a presence of an acceleration disc around its huge black hole. This in turn, emits strong radiation and ultraviolet rays that later get ejected into the depths of space.

References

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  1. ^ "NGC 5940 - Spiral Galaxy in | TheSkyLive.com". theskylive.com. Retrieved 2024-04-16.
  2. ^ a b c "New General Catalog Objects: NGC 5900 - 5949". cseligman.com. Retrieved 2024-04-16.
  3. ^ a b "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-04-16.
  4. ^ Adegoke, Oluwashina K. (May 2022). "XMM-Newton and Swift Observations of the Seyfert 1 AGN NGC 5940". Astrophysics and Space Science. 367 (5): 51. arXiv:2205.11612. Bibcode:2022Ap&SS.367...51A. doi:10.1007/s10509-022-04082-1. ISSN 0004-640X.
  5. ^ "NGC 5940". simbad.u-strasbg.fr. Retrieved 2024-04-16.
  6. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-16.