NGC 3610

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NGC 3610
NIR)
Other designations
NGC 3610, UGC 6319, LEDA 34566, PGC 34566[5]

NGC 3610 is an

Ursa Major.[6] It was discovered on 8 April 1793 by German-British astronomer William Herschel.[7] This galaxy is located at a distance of 106 million light-years (32.5 Mpc) from the Milky Way,[4] and is receding with a galacto-centric radial velocity of 1,819 km/s.[3]

NGC 3610 is a relatively young elliptical galaxy which has not yet lost its disk.

major and minor axes of the elliptical profile. This is a candidate merger remnant of intermediate age, with a surviving disk of gas and dusk aligned with the major axis.[9] This merger is estimated to have occurred 4±2.5 Gyr ago. The central part of the disk displays warping,[8] and is significantly younger than the remainder of the galaxy.[8]

The unusual amount of blue light emission of NGC 3610, or B–V in the UBV photometric system, suggests recent star formation.[9] The current estimated star formation rate is 0.385±0.375 M·yr−1.[4] There is a population of younger globular clusters orbiting the galaxy that is a likely product of the merger. The surviving population of older, metal-rich globular clusters suggests that at least one of the progenitor galaxies had a prominent bulge component.[9]

Gallery

References

  1. ^
    S2CID 18913331
    .
  2. ^ a b c "Results for NGC 252". NASA/IPAC Extragalactic Database. Retrieved 12 February 2017.
  3. ^
    S2CID 250737862
    .
  4. ^ .
  5. ^ "NGC 3610". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 12 February 2017.
  6. ^ a b "A young elliptical". Hubble Space Telescope. Retrieved 16 December 2016.
  7. ^ Seligman, Courtney. "NGC 3610 (= PGC 34566)". cseligman. Retrieved 12 February 2017.
  8. ^ .
  9. ^ .

Further reading

External links

  • Media related to NGC 3610 at Wikimedia Commons