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The three galaxies involved in the interaction, are PGC 84569 or known as SBS 1520+503 and IRAS 15205+5021,[4] 2MASX J15220246+5010185 or PGC 3845255[5] and SDSS J152202.25+501027.9 or PGC 4530597.[6] All of them have distorted appearances with strands of dust and gas running between them.[7] It is also likely that their interactions cause periods of extreme star formation thus making it into an luminous infrared galaxy.[8] SDSSCGB 10189 is set on a collision course, in which the result will be a single larger galaxy.[7]
This trio is an exceptionally rare combination in the close proximity of each of the galaxies to one another: they are lying only 50,000 light-years apart from one another to the point they are considered close galactic neighbors.[7] To the left of the interacting trio, a foreground dimmer spiral galaxy called PGC 2365567[9] is located which appears to float serenely along the collision.[7]
This observation was conducted to help astronomers understand the origin of massive galaxies. They are called brightest cluster galaxies and suspected they can be formed through merging of large gas-rich galaxies.[7] By looking at SDSSCGB 10189, it shows how galaxies undergo changes through merging and transform over time from disk galaxies to spheroids.[10][11]
^Martin, G.; Kaviraj, S.; Devriendt, J. E. G.; Dubois, Y.; Pichon, C. (2018-10-21). "The role of mergers in driving morphological transformation over cosmic time". Monthly Notices of the Royal Astronomical Society. 480 (2): 2266–2283. arXiv:1807.08761. doi:10.1093/mnras/sty1936. ISSN0035-8711.
This page was last edited on 16 May 2024, at 00:36