ESO 69-6 explained

ESO 69-6
Constellation Name:Triangulum Australe
Z:0.046439
H Radial V:14,082 km/s
Dist Ly:654 Mly (200.6 Mpc)
Appmag V:16.16
Type:LIRG
Notes:Interacting galaxies
Names:ESO 069-IG 006, PGC 58663, AM 1633-682, 2MASX J16381190-6826080, IRAS 16330-6820, 2MASS J16381342-6827167, CXO J163813.4-682717
Epoch:J2000

ESO 69-6 collectively known as AM 1633-682,[1] is a pair of interacting galaxies located 654 million light-years away in the constellation of Triangulum Australe. They are made of two galaxies: ESO 069-IG 006N known as IRAS 16330-6820,[2] and ESO 069-IG 006S known as LEDA 285730.[3]

Characteristics

Both galaxies are in stages of merging with each other.[4] They resemble musical notes on a stave.[5] Long tidal tails are formed, which stars and gas are stripped and torn away from their outer regions.[6] These tails are proven signs of their interactions. Additionally numerical simulations that reproduces interaction-induced inflow of gas and resulting nuclear starbursts can, might trigger strong starbursts in both galaxies.[7]

It is proven from the gravitational interactions of ESO 69–6, the surrounding intergalactic medium can be enriched with metals very efficiently up to distances of several 100 kpc.[8] This can be explained in terms of indirect processes or direct processes that create kinetic spreading of baryonic matter. Possibly, they will eventually merge with each other and form a much bigger galaxy, in this case an elliptical galaxy, in the future.[9] [10]

References

  1. Web site: Your NED Search Results . 2024-04-29 . ned.ipac.caltech.edu.
  2. Web site: NED Search Results for ESO 069-IG 006N . 2024-04-29 . ned.ipac.caltech.edu.
  3. Web site: NED Search Results for ESO 069-IG 006S . 2024-04-29 . ned.ipac.caltech.edu.
  4. Web site: Galaxies - Merging and Interacting Center for Astrophysics Harvard & Smithsonian . 2024-04-29 . www.cfa.harvard.edu.
  5. Web site: information@eso.org . ESO 69-6 . 2024-04-29 . www.spacetelescope.org . en.
  6. 1993MNRAS.263..349S Page 349 . 2024-04-29 . adsabs.harvard.edu. 1993MNRAS.263..349S .
  7. Web site: Star formation in galaxy interactions and mergers - Frederic Bournaud . 2024-04-29 . ned.ipac.caltech.edu.
  8. Kapferer . W. . Knapp . A. . Schindler . S. . Kimeswenger . S. . Kampen . E. van . 2005-07-01 . Star formation rates and mass distributions in interacting galaxies . Astronomy & Astrophysics . en . 438 . 1 . 87–101 . 10.1051/0004-6361:20052753 . astro-ph/0503559 . 2005A&A...438...87K . 0004-6361.
  9. Chatterjee . Tapan K. . 1993-01-01 . Interacting galaxies and mergers . Astrophysics and Space Science . en . 199 . 2 . 189–197 . 10.1007/BF00613194 . 1993Ap&SS.199..189C . 1572-946X.
  10. Chou . Richard C. . American Astronomical Society, AAS Meeting #219, Id.411.04 . 2012-01-01 . Observational Studies of Interacting Galaxies and the Development of a Wide Integral-field Infrared Spectrograph . 219 . 411.04. 2012AAS...21941104C .