Galaxybeing: Created SDSSCGB 10189
{{Infobox galaxy|name=SDSSCGB 10189|image=File
otw2307a.jpg|caption=[[Hubble]] image of SDSSCGB 10189|constellation name=[[Boötes (constellation)|Boötes]]|ra=230.50 degree|dec=50.17 degree|z=0.074000|h_radial_v=21,310 km/s|dist_ly=1.045 Gly (320.4 M[[Parsec|pc]])|notes=[[Interacting galaxies]]|names=SDSSCGB 10189, [[IRAS]] 15205+5021, MLCG 1320, [[2MASS]] J15220252+5010189, [[2MASX]] J152200246+5010185, [[Principal Galaxies Catalogue|PGC]] 84569, [[NRAO VLA Sky Survey|NVSS]] J152201+5010030, SBS 1520+503, [[Sloan Digital Sky Survey|SDSS]] J152201.60+501028.6}}
'''SDSSCGB 10189''' are a trio of [[Galaxy|galaxies]] located in the constellation of [[Boötes]].<ref>{{Cite web |last=Guide |first=Universe |date=19-02-2023T21:00:46 |title=SDSS CGB 10189 Facts |url=https://www.universeguide.com/galaxy/sdsscgb-10189 |access-date=2024-04-29 |website=Universe Guide |language=en-us}}</ref> They are located 1.04 billion [[Light-year|light-years]] away from the [[Solar System|solar system]]<ref>{{Cite web |title=Your NED Search Results |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-04-29 |website=ned.ipac.caltech.edu}}</ref> and are [[Gravity|gravitationally]] [[Interacting galaxy|interacting]].<ref>{{Cite web |title=Galaxies - Merging and Interacting {{!}} Center for Astrophysics {{!}} Harvard & Smithsonian |url=https://www.cfa.harvard.edu/research/topic/galaxies-merging-and-interacting |access-date=2024-04-29 |website=www.cfa.harvard.edu}}</ref>
== Characteristics ==
The three galaxies involved in the interaction, are PGC 84569 or known as SBS 1520+503 and IRAS 15205+5021<ref>{{Cite web |title=HyperLeda -object description for PGC 84569 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=PGC 84569 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref>, 2MASX J15220246+5010185 or PGC 3845255<ref>{{Cite web |title=HyperLeda -object description for 2MASX J15220246+5010185 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=SDSSCGB 10189 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref> and SDSS J152202.25+501027.9 or PGC 4530597.<ref>{{Cite web |title=HyperLeda -object description for SDSS J152202.25+501027.9 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=SDSSCGB 10189 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref> All of them have distorted appearances with strands of dust and gas running between them.<ref name=":0">{{Cite web |last=information@eso.org |title=Galactic Crash Course |url=https://www.spacetelescope.org/images/potw2307a/ |access-date=2024-04-29 |website=www.spacetelescope.org |language=en}}</ref> It is also likely that their interactions cause periods of extreme [[star formation]] thus making it into an [[luminous infrared galaxy]].<ref>{{Cite journal |last=Pearson |first=W. J. |last2=Wang |first2=L. |last3=Alpaslan |first3=M. |last4=Baldry |first4=I. |last5=Bilicki |first5=M. |last6=Brown |first6=M. J. I. |last7=Grootes |first7=M. W. |last8=Holwerda |first8=B. W. |last9=Kitching |first9=T. D. |last10=Kruk |first10=S. |last11=Tak |first11=F. F. S. van der |date=2019-11-01 |title=Effect of galaxy mergers on star-formation rates |url=https://www.aanda.org/articles/aa/abs/2019/11/aa36337-19/aa36337-19.html |journal=Astronomy & Astrophysics |language=en |volume=631 |pages=A51 |doi=10.1051/0004-6361/201936337 |issn=0004-6361}}</ref> SDSSCGB 10189 is set on a collision course, in which the result will be a [[Elliptical galaxy|single larger galaxy]].<ref name=":0" />
This trio is an exceptionally rare combination as it is a surprise they are lying only 50,000 thousand light-years from each other to the point they are considered close galactic neighbors.<ref name=":0" /> To the left of the interacting trio, a foreground dimmer [[spiral galaxy]] called PGC 2365567<ref>{{Cite web |title=HyperLeda -object description for PGC 2365567 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=SDSSCGB 10189 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref> is located which appears to float serenely along the collision.<ref name=":0" />
This observation was conducted to help [[Astronomer|astronomers]] understand the origin of massive galaxies. They are called [[Brightest cluster galaxy|brightest cluster galaxies]] and suspected they can be formed through merging of large [[Interstellar medium|gas-rich]] galaxies.<ref name=":0" /> By looking at SDSSCGB 10189, it shows how galaxies undergo changes through merging and transform over time from [[Disc galaxy|disk galaxies]] to [[Spheroid|spheroids]].<ref>{{Cite web |last=Nguyen |first=Thinh |title=Alchemy of Galaxies – How galaxies merge and transform over time |url=https://astrobites.org/2023/07/05/alchemy-of-galaxies-how-galaxies-merge-and-transform-over-time/ |access-date=2024-04-29 |website=Astrobites}}</ref><ref>{{Cite journal |last=Martin |first=G. |last2=Kaviraj |first2=S. |last3=Devriendt |first3=J. E. G. |last4=Dubois |first4=Y. |last5=Pichon |first5=C. |date=2018-10-21 |title=The role of mergers in driving morphological transformation over cosmic time |url=http://arxiv.org/abs/1807.08761 |journal=Monthly Notices of the Royal Astronomical Society |volume=480 |issue=2 |pages=2266–2283 |doi=10.1093/mnras/sty1936 |issn=0035-8711}}</ref>
== References ==
<references />
[[Category:Boötes]]
[[Category:Interacting galaxies]]
[[Category:IRAS catalogue objects]]
[[Category:Luminous infrared galaxies]]
[[Category:SDSS objects]]
[[Category:2MASS objects]]
[[Categoryrincipal Galaxies Catalogue objects]]
Okumaya devam et...
{{Infobox galaxy|name=SDSSCGB 10189|image=File
otw2307a.jpg|caption=[[Hubble]] image of SDSSCGB 10189|constellation name=[[Boötes (constellation)|Boötes]]|ra=230.50 degree|dec=50.17 degree|z=0.074000|h_radial_v=21,310 km/s|dist_ly=1.045 Gly (320.4 M[[Parsec|pc]])|notes=[[Interacting galaxies]]|names=SDSSCGB 10189, [[IRAS]] 15205+5021, MLCG 1320, [[2MASS]] J15220252+5010189, [[2MASX]] J152200246+5010185, [[Principal Galaxies Catalogue|PGC]] 84569, [[NRAO VLA Sky Survey|NVSS]] J152201+5010030, SBS 1520+503, [[Sloan Digital Sky Survey|SDSS]] J152201.60+501028.6}}'''SDSSCGB 10189''' are a trio of [[Galaxy|galaxies]] located in the constellation of [[Boötes]].<ref>{{Cite web |last=Guide |first=Universe |date=19-02-2023T21:00:46 |title=SDSS CGB 10189 Facts |url=https://www.universeguide.com/galaxy/sdsscgb-10189 |access-date=2024-04-29 |website=Universe Guide |language=en-us}}</ref> They are located 1.04 billion [[Light-year|light-years]] away from the [[Solar System|solar system]]<ref>{{Cite web |title=Your NED Search Results |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-04-29 |website=ned.ipac.caltech.edu}}</ref> and are [[Gravity|gravitationally]] [[Interacting galaxy|interacting]].<ref>{{Cite web |title=Galaxies - Merging and Interacting {{!}} Center for Astrophysics {{!}} Harvard & Smithsonian |url=https://www.cfa.harvard.edu/research/topic/galaxies-merging-and-interacting |access-date=2024-04-29 |website=www.cfa.harvard.edu}}</ref>
== Characteristics ==
The three galaxies involved in the interaction, are PGC 84569 or known as SBS 1520+503 and IRAS 15205+5021<ref>{{Cite web |title=HyperLeda -object description for PGC 84569 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=PGC 84569 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref>, 2MASX J15220246+5010185 or PGC 3845255<ref>{{Cite web |title=HyperLeda -object description for 2MASX J15220246+5010185 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=SDSSCGB 10189 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref> and SDSS J152202.25+501027.9 or PGC 4530597.<ref>{{Cite web |title=HyperLeda -object description for SDSS J152202.25+501027.9 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=SDSSCGB 10189 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref> All of them have distorted appearances with strands of dust and gas running between them.<ref name=":0">{{Cite web |last=information@eso.org |title=Galactic Crash Course |url=https://www.spacetelescope.org/images/potw2307a/ |access-date=2024-04-29 |website=www.spacetelescope.org |language=en}}</ref> It is also likely that their interactions cause periods of extreme [[star formation]] thus making it into an [[luminous infrared galaxy]].<ref>{{Cite journal |last=Pearson |first=W. J. |last2=Wang |first2=L. |last3=Alpaslan |first3=M. |last4=Baldry |first4=I. |last5=Bilicki |first5=M. |last6=Brown |first6=M. J. I. |last7=Grootes |first7=M. W. |last8=Holwerda |first8=B. W. |last9=Kitching |first9=T. D. |last10=Kruk |first10=S. |last11=Tak |first11=F. F. S. van der |date=2019-11-01 |title=Effect of galaxy mergers on star-formation rates |url=https://www.aanda.org/articles/aa/abs/2019/11/aa36337-19/aa36337-19.html |journal=Astronomy & Astrophysics |language=en |volume=631 |pages=A51 |doi=10.1051/0004-6361/201936337 |issn=0004-6361}}</ref> SDSSCGB 10189 is set on a collision course, in which the result will be a [[Elliptical galaxy|single larger galaxy]].<ref name=":0" />
This trio is an exceptionally rare combination as it is a surprise they are lying only 50,000 thousand light-years from each other to the point they are considered close galactic neighbors.<ref name=":0" /> To the left of the interacting trio, a foreground dimmer [[spiral galaxy]] called PGC 2365567<ref>{{Cite web |title=HyperLeda -object description for PGC 2365567 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=SDSSCGB 10189 |access-date=2024-04-29 |website=atlas.obs-hp.fr}}</ref> is located which appears to float serenely along the collision.<ref name=":0" />
This observation was conducted to help [[Astronomer|astronomers]] understand the origin of massive galaxies. They are called [[Brightest cluster galaxy|brightest cluster galaxies]] and suspected they can be formed through merging of large [[Interstellar medium|gas-rich]] galaxies.<ref name=":0" /> By looking at SDSSCGB 10189, it shows how galaxies undergo changes through merging and transform over time from [[Disc galaxy|disk galaxies]] to [[Spheroid|spheroids]].<ref>{{Cite web |last=Nguyen |first=Thinh |title=Alchemy of Galaxies – How galaxies merge and transform over time |url=https://astrobites.org/2023/07/05/alchemy-of-galaxies-how-galaxies-merge-and-transform-over-time/ |access-date=2024-04-29 |website=Astrobites}}</ref><ref>{{Cite journal |last=Martin |first=G. |last2=Kaviraj |first2=S. |last3=Devriendt |first3=J. E. G. |last4=Dubois |first4=Y. |last5=Pichon |first5=C. |date=2018-10-21 |title=The role of mergers in driving morphological transformation over cosmic time |url=http://arxiv.org/abs/1807.08761 |journal=Monthly Notices of the Royal Astronomical Society |volume=480 |issue=2 |pages=2266–2283 |doi=10.1093/mnras/sty1936 |issn=0035-8711}}</ref>
== References ==
<references />
[[Category:Boötes]]
[[Category:Interacting galaxies]]
[[Category:IRAS catalogue objects]]
[[Category:Luminous infrared galaxies]]
[[Category:SDSS objects]]
[[Category:2MASS objects]]
[[Category
rincipal Galaxies Catalogue objects]]Okumaya devam et...