South America Galaxy

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South America Galaxy
A very bright contortionist.jpg
The galaxy, as seen by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Aquarius
Right ascension 22h 51m 49.2s
Declination −17° 52′ 23″
Redshift 0.077750
Heliocentric radial velocity 23,309 km/s
Distance 1.045 Gly (320.4 Mpc)
Apparent magnitude  (B)16.15
Characteristics
Type LIG
Size90,000 ly (estimated)
Apparent size  (V)0.3' x 0.2'
Notable features Interacting galaxies
Other designations
LEDA 69877, IRAS 22491-1808, PGC 69877, NVSS J225149-175225

The South America Galaxy, also known as LEDA 69877 and IRAS 22491-1808, is a merging pair of ultraluminous infrared galaxies located in the constellation Aquarius. [1] [2] It is estimated to be 1.045 billion light-years from the Milky Way and about 90,000 light-years in diameter. The object is moving away from the Solar System with a calculated radial velocity of approximately 23.300 kilometers per second. [3]

Contents

The galaxy got its nickname due to its physical resemblance to the continent of South America. The galaxy was selected as ESA/HUBBLE's picture of the week on 10 June 2013. [4]

In the complex central region of the galaxy, scientists have been able to distinguish two nuclei, remains of the two different galaxies that are currently colliding. IRAS 22491-1808 is among the most luminous of these types of galaxies, and is considered to be mid-way through its merging stage. [4]

According to a study published in 2017, the mass of the molecular gas outflow in IRAS 22491-1808 is estimated to be MH2(hot)~ 6−8 × 103M. [5] Notable, it also shows lack of polarization. [6]

See also

References

  1. Braito, V.; Franceschini, A.; Della Ceca, R.; Bassani, L.; Cappi, M.; Malaguti, P.; Palumbo, G. G. C.; Persic, M.; Risaliti, G. (2002-02-19). "An XMM-Newton Survey of Ultra-Luminous Infrared Galaxies". arXiv: astro-ph/0202352 .
  2. Sanders, D. B.; Mirabel, I. F. (1996-01-01). "Luminous Infrared Galaxies". Annual Review of Astronomy and Astrophysics. 34 (1): 749. Bibcode:1996ARA&A..34..749S. doi:10.1146/annurev.astro.34.1.749. ISSN   0066-4146.
  3. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-07-23.
  4. 1 2 information@eso.org. "A very bright contortionist". esahubble.org. Retrieved 2024-07-23.
  5. Emonts, B. H. C.; Colina, L.; Piqueras-López, J.; Garcia-Burillo, S.; Pereira-Santaella, M.; Arribas, S.; Labiano, A.; Alonso-Herrero, A. (2017-11-01). "Outflows of hot molecular gas in ultra-luminous infrared galaxies mapped with VLT-SINFONI". Astronomy & Astrophysics. 607: A116. arXiv: 1708.09503 . Bibcode:2017A&A...607A.116E. doi:10.1051/0004-6361/201731508. ISSN   0004-6361.
  6. Pernechele, C.; Berta, S.; Marconi, A.; Bonoli, C.; Bressan, A.; Franceschini, A.; Fritz, J.; Giro, E. (2003-01-01). "Spectropolarimetric search for hidden active galactic nuclei in four southern ultraluminous infrared galaxies". Monthly Notices of the Royal Astronomical Society. 338 (1): L13 –L17. arXiv: astro-ph/0210690 . Bibcode:2003MNRAS.338L..13P. doi: 10.1046/j.1365-8711.2003.06112.x . ISSN   0035-8711.