Galaxybeing: Created 2MASX J09133888-1019196
{{Infobox galaxy|name=2MASX J09133888-1019196|image=Hubble Interacting Galaxy 2MASX J09133888-1019196 (2008-04-24).jpg|caption=[[Hubble Space Telescope]] image of 2MASX J09133888-1019196|constellation name=[[Hydra (constellation)|Hydra]]|ra=138.41 degree|dec=-10.32 degree|z=0.054141|h_radial_v=16,500 km/s|dist_ly=735 [[Mly]] (225.35 Mpc)|appmag_v=15.9|type=HII, LIRG, S2|notes=[[Luminous Infrared Galaxy]]|names=[[IRAS]] 09111-1007, [[6dF]] J0913389-101920, [[2MASS]] J09133883-1019200, [[Principal Galaxies Catalogue|PGC]] 153577, LQAC 138-010 001, NPM1G -10.0288, [[IRAS]] 09111-1007E, 2CXO J091338.8-101919, [[Lyon-Meudon Extragalactic Database|LEDA]] 153577}}
'''2MASX J09133888-1019196''' are a pair of [[Interacting galaxy|interacting galaxies]] located in the constellation of [[Hydra (constellation)|Hydra]].<ref name=":0">{{Cite web |title=Hubble Interacting Galaxy 2MASX J09133888-1019196 |url=https://hubblesite.org/contents/media/images/2008/16/2304-Image.html |website=Hubblesite}}</ref> It is located 735 million [[Light-year|light-years]] 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=2024-04-28 |website=ned.ipac.caltech.edu}}</ref>
== Characteristics ==
2MASX J09133888-1019196 has a distorted appearance due to the gravity interactions and there is a gap distance of 130,000 thousand light-years between the galaxies, meaning they are beginning to merge.<ref name=":0" /> 2MASX J09133888-1019196 is considered as a [[luminous infrared galaxy]]<ref>{{Citation |last=Lonsdale |first=Carol |title=Ultraluminous Infrared Galaxies |date=2006 |pages=285–336 |url=http://arxiv.org/abs/astro-ph/0603031 |access-date=2024-04-28 |last2=Farrah |first2=Duncan |last3=Smith |first3=Harding}}</ref> which is unusual for such early stages of interacting galaxies.<ref name=":0" /><ref>{{Cite web |title=Morphological classification of local luminous infrared galaxies {{!}} Astronomy & Astrophysics (A&A) |url=https://www.aanda.org/articles/aa/full_html/2016/07/aa28093-16/T2.html?mb=0 |access-date=2024-04-28 |website=www.aanda.org |language=en-gb}}</ref> It is possibly powered by [[Starburst galaxy|starbursts]] with high [[star formation]] rates, exceeding 100 ''M''⊙ yr−1, that is combined with contribution from an [[active galactic nucleus]].<ref>{{Cite journal |last=Abbasi |first=R. |last2=Ackermann |first2=M. |last3=Adams |first3=J. |last4=Aguilar |first4=J. A. |last5=Ahlers |first5=M. |last6=Ahrens |first6=M. |last7=Alispach |first7=C. |last8=Alves |first8=A. A. |last9=Amin |first9=N. M. |last10=An |first10=R. |last11=Andeen |first11=K. |last12=Anderson |first12=T. |last13=Anton |first13=G. |last14=Argüelles |first14=C. |last15=Ashida |first15=Y. |date=2022-02 |title=Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |url=https://dx.doi.org/10.3847/1538-4357/ac3cb6 |journal=The Astrophysical Journal |language=en |volume=926 |issue=1 |pages=59 |doi=10.3847/1538-4357/ac3cb6 |issn=0004-637X}}</ref> It is also likely that one or both galaxies might have experienced merging or interacted in the past. Both galaxies have [[Supermassive black hole|supermassive black holes]] lurking in their cores.<ref name=":0" /> According to [[SIMBAD]], 2MASX J09133888-1019196 is described as [[Seyfert galaxy|Seyfert]] 2 galaxy<ref>{{Cite web |title=2MASX J09133888-1019196 |url=https://simbad.u-strasbg.fr/simbad/sim-basic |access-date=2024-04-28 |website=simbad.u-strasbg.fr}}</ref>, hence its reason for having high luminosity.
== References ==
<references />
[[Category:Interacting galaxies]]
[[Category:Hydra (constellation)]]
[[Category:Luminous infrared galaxies]]
[[Category:2MASS objects]]
[[Category
rincipal Galaxies Catalogue objects]]
[[Category:Seyfert galaxies]]
[[Category:LEDA objects]]
[[Category:IRAS catalogue objects]]
Okumaya devam et...
{{Infobox galaxy|name=2MASX J09133888-1019196|image=Hubble Interacting Galaxy 2MASX J09133888-1019196 (2008-04-24).jpg|caption=[[Hubble Space Telescope]] image of 2MASX J09133888-1019196|constellation name=[[Hydra (constellation)|Hydra]]|ra=138.41 degree|dec=-10.32 degree|z=0.054141|h_radial_v=16,500 km/s|dist_ly=735 [[Mly]] (225.35 Mpc)|appmag_v=15.9|type=HII, LIRG, S2|notes=[[Luminous Infrared Galaxy]]|names=[[IRAS]] 09111-1007, [[6dF]] J0913389-101920, [[2MASS]] J09133883-1019200, [[Principal Galaxies Catalogue|PGC]] 153577, LQAC 138-010 001, NPM1G -10.0288, [[IRAS]] 09111-1007E, 2CXO J091338.8-101919, [[Lyon-Meudon Extragalactic Database|LEDA]] 153577}}
'''2MASX J09133888-1019196''' are a pair of [[Interacting galaxy|interacting galaxies]] located in the constellation of [[Hydra (constellation)|Hydra]].<ref name=":0">{{Cite web |title=Hubble Interacting Galaxy 2MASX J09133888-1019196 |url=https://hubblesite.org/contents/media/images/2008/16/2304-Image.html |website=Hubblesite}}</ref> It is located 735 million [[Light-year|light-years]] 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=2024-04-28 |website=ned.ipac.caltech.edu}}</ref>
== Characteristics ==
2MASX J09133888-1019196 has a distorted appearance due to the gravity interactions and there is a gap distance of 130,000 thousand light-years between the galaxies, meaning they are beginning to merge.<ref name=":0" /> 2MASX J09133888-1019196 is considered as a [[luminous infrared galaxy]]<ref>{{Citation |last=Lonsdale |first=Carol |title=Ultraluminous Infrared Galaxies |date=2006 |pages=285–336 |url=http://arxiv.org/abs/astro-ph/0603031 |access-date=2024-04-28 |last2=Farrah |first2=Duncan |last3=Smith |first3=Harding}}</ref> which is unusual for such early stages of interacting galaxies.<ref name=":0" /><ref>{{Cite web |title=Morphological classification of local luminous infrared galaxies {{!}} Astronomy & Astrophysics (A&A) |url=https://www.aanda.org/articles/aa/full_html/2016/07/aa28093-16/T2.html?mb=0 |access-date=2024-04-28 |website=www.aanda.org |language=en-gb}}</ref> It is possibly powered by [[Starburst galaxy|starbursts]] with high [[star formation]] rates, exceeding 100 ''M''⊙ yr−1, that is combined with contribution from an [[active galactic nucleus]].<ref>{{Cite journal |last=Abbasi |first=R. |last2=Ackermann |first2=M. |last3=Adams |first3=J. |last4=Aguilar |first4=J. A. |last5=Ahlers |first5=M. |last6=Ahrens |first6=M. |last7=Alispach |first7=C. |last8=Alves |first8=A. A. |last9=Amin |first9=N. M. |last10=An |first10=R. |last11=Andeen |first11=K. |last12=Anderson |first12=T. |last13=Anton |first13=G. |last14=Argüelles |first14=C. |last15=Ashida |first15=Y. |date=2022-02 |title=Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube |url=https://dx.doi.org/10.3847/1538-4357/ac3cb6 |journal=The Astrophysical Journal |language=en |volume=926 |issue=1 |pages=59 |doi=10.3847/1538-4357/ac3cb6 |issn=0004-637X}}</ref> It is also likely that one or both galaxies might have experienced merging or interacted in the past. Both galaxies have [[Supermassive black hole|supermassive black holes]] lurking in their cores.<ref name=":0" /> According to [[SIMBAD]], 2MASX J09133888-1019196 is described as [[Seyfert galaxy|Seyfert]] 2 galaxy<ref>{{Cite web |title=2MASX J09133888-1019196 |url=https://simbad.u-strasbg.fr/simbad/sim-basic |access-date=2024-04-28 |website=simbad.u-strasbg.fr}}</ref>, hence its reason for having high luminosity.
== References ==
<references />
[[Category:Interacting galaxies]]
[[Category:Hydra (constellation)]]
[[Category:Luminous infrared galaxies]]
[[Category:2MASS objects]]
[[Category
rincipal Galaxies Catalogue objects]][[Category:Seyfert galaxies]]
[[Category:LEDA objects]]
[[Category:IRAS catalogue objects]]
Okumaya devam et...