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{{Infobox galaxy|name=IC 1182|image=File:IC1182 - SDSS DR14.jpg|caption=[[Sloan Digital Sky Survey|SDSS]] image of IC 1182|constellation name=[[Hercules (constellation)|Hercules]]|ra=241.40 degree|dec=17.80 degree|z=0.034210|h_radial_v=10,206 km/s|dist_ly=464 Mly (142.26 M[[Parsec|pc]])|appmag_v=15.19|type=SAO+ pec, HII|size=135,000 ly|names=[[Principal Galaxies Catalogue|PGC]] 57084, [[Uppsala General Catalogue|UGC]] 10192, [[Catalogue of Galaxies and of Clusters of Galaxies|CGCG]] 108-126, [[Morphological Catalogue of Galaxies|MCG]] +03-41-104, [[Markarian galaxies|Mrk]] 298, AGC 260184, NPM1G+17.0584, [[2MASX]] J16053680+1748078, [[NRAO VLA Sky Survey|NVSS]] J160536+174804, 1RXS J160537.9+174740, KUG 1603+179B, [[Sloan Digital Sky Survey|SDSS]] J160536.78+174807.5, WBL 607-016, [[2MASS]] J16053680+1748075, [[Lyon-Meudon Extragalactic Database|LEDA]] 57084|group_cluster=[[Hercules Cluster]]}}
'''IC 1182''' is a type S0-a<ref>{{Cite web |title=HyperLeda -object description |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=IC 1182 |access-date=2024-04-30 |website=atlas.obs-hp.fr}}</ref> [[lenticular galaxy]] located in [[Hercules (constellation)|Hercules]].<ref>{{Cite web |last=Ford |first=Dominic |title=IC1182 (Galaxy) |url=https://in-the-sky.org//data/object.php?id=IC1182 |access-date=2024-04-30 |website=In-The-Sky.org |language=en}}</ref> It is located 464 million [[Light-year|light-years]] away from the [[Solar System|solar system]]<ref name=":0">{{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=2024-04-30 |website=ned.ipac.caltech.edu}}</ref> and was discovered on August 11, 1892 by [[Stéphane Javelle|Stephane Javelle]].<ref>{{Cite web |title=Index Catalog Objects: IC 1150 - 1199 |url=https://cseligman.com/text/atlas/ic11a.htm#ic1182 |access-date=2024-04-30 |website=cseligman.com}}</ref> IC 1198 is a member of the [[Hercules Cluster]],<ref name=":0" /> which is a part of the [[CfA2 Great Wall|CfA 2 Great Wall]].<ref>{{Cite web |title=Clusters and Superclusters of Galaxies |url=https://ned.ipac.caltech.edu/level5/Sept01/Bahcall2/Bahcall9_2.html |access-date=2024-04-30 |website=ned.ipac.caltech.edu}}</ref>
== Description ==
IC 1182 was originally classified as a [[Seyfert galaxy|Seyfert]] type 2 galaxy but later, research proves, it is indeed an unusual and rare galaxy in some kind of merger event.<ref>{{Cite web |title=Object of the Week May 25, 2014 IC 1182 A Member of The Jet Set |url=https://www.deepskyforum.com/showth...k-May-25-2014-IC-1182-A-Member-of-The-Jet-Set |access-date=2024-04-30 |website=www.deepskyforum.com}}</ref> It presents a [[Astrophysical jet|jet]] that is extending out from the center in east direction comprising of [[Kinetic energy|kinetic material]].<ref name=":1">{{Cite web |last=information@eso.org |title=The VLT Records Faint Structures in Colliding Galaxies |url=https://www.eso.org/public/news/eso9834/ |access-date=2024-04-30 |website=www.eso.org |language=es}}</ref> There is a broad faint S-shaped plume and debris on the other side of the galaxy. Not to mention, IC 1182 radiates a lot of [[energy]] and expels a subsential amount of material at high [[velocity]] into depths of space. In its central region, clusters of [[O-type main-sequence star|O-type]] hot blue stars are present.<ref name=":1" />
== An ongoing merger? ==
IC 1182 shows high resolution broad and narrow band images and long slit [[spectroscopy]]. It reveals a distorted morphology with a heavily [[Interstellar cloud|obscured disk-link structure]] with several knots in its regions.<ref name=":2">{{Cite journal |last=Moles |first=M. |last2=Bettoni |first2=D. |last3=Fasano |first3=G. |last4=Kjærgaard |first4=P. |last5=Varela |first5=J. |last6=Milvang-Jensen |first6=B. |date=2004-05-01 |title=The peculiar galaxy IC 1182: An ongoing merger? |url=https://www.aanda.org/articles/aa/abs/2004/17/aa0295/aa0295.html |journal=Astronomy & Astrophysics |language=en |volume=418 |issue=2 |pages=495–507 |doi=10.1051/0004-6361:20034295 |issn=0004-6361}}</ref> Some of the [[Interstellar medium|galactic material]], in the form of two slender tails are detected beyond the main body of the [[galaxy]]. IC 1182 has [[Color index|color indices]] of an early type object which is significantly bluer than what is typical for the kind of galaxy.<ref name=":2" /> The [[Narrow-line region|narrow lines]] shows this galaxy is a [[Active galactic nucleus|powerful emitter]] which the knots in the central region and inside the tail emerging eastward from the galaxy are [[Luminous efficacy|luminous]] in H''α'' and have typical sizes of 1 kpc.<ref name=":2" />
Additionally, IC 1182 presents large quantities of neural [[hydrogen]] which its distance-independent ratio of hydrogen mass to optical luminosity is equal to 0.7 times the [[Solar radio emission|solar ratio]].<ref name=":3">{{Cite journal |last=Bothun |first=G. D. |last2=Stauffer |first2=J. R. |last3=Schommer |first3=R. A. |date=1981-07-01 |title=The peculiar galaxy IC 1182. |url=https://ui.adsabs.harvard.edu/abs/1981ApJ...247...42B |journal=The Astrophysical Journal |volume=247 |pages=42–47 |doi=10.1086/159007 |issn=0004-637X}}</ref> This might be indicated, it might be in a collision involving a gas-rich spiral which gives rise to observed nuclear [[Spectral line|emission lines]]. <ref name=":3" />
== References ==
<references />
[[Category:IC objects]]
[[Category:UGC objects]]
[[Category:Markarian galaxies]]
[[Category
rincipal Galaxies Catalogue objects]]
[[Category:Astronomical objects discovered in 1892]]
[[Category:Hercules (constellation)]]
[[Category:LEDA objects]]
[[Category:SDSS objects]]
[[Category:2MASS objects]]
[[Category:Lenticular galaxies]]
[[Category:Hercules Cluster]]
Okumaya devam et...
{{Infobox galaxy|name=IC 1182|image=File:IC1182 - SDSS DR14.jpg|caption=[[Sloan Digital Sky Survey|SDSS]] image of IC 1182|constellation name=[[Hercules (constellation)|Hercules]]|ra=241.40 degree|dec=17.80 degree|z=0.034210|h_radial_v=10,206 km/s|dist_ly=464 Mly (142.26 M[[Parsec|pc]])|appmag_v=15.19|type=SAO+ pec, HII|size=135,000 ly|names=[[Principal Galaxies Catalogue|PGC]] 57084, [[Uppsala General Catalogue|UGC]] 10192, [[Catalogue of Galaxies and of Clusters of Galaxies|CGCG]] 108-126, [[Morphological Catalogue of Galaxies|MCG]] +03-41-104, [[Markarian galaxies|Mrk]] 298, AGC 260184, NPM1G+17.0584, [[2MASX]] J16053680+1748078, [[NRAO VLA Sky Survey|NVSS]] J160536+174804, 1RXS J160537.9+174740, KUG 1603+179B, [[Sloan Digital Sky Survey|SDSS]] J160536.78+174807.5, WBL 607-016, [[2MASS]] J16053680+1748075, [[Lyon-Meudon Extragalactic Database|LEDA]] 57084|group_cluster=[[Hercules Cluster]]}}
'''IC 1182''' is a type S0-a<ref>{{Cite web |title=HyperLeda -object description |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=IC 1182 |access-date=2024-04-30 |website=atlas.obs-hp.fr}}</ref> [[lenticular galaxy]] located in [[Hercules (constellation)|Hercules]].<ref>{{Cite web |last=Ford |first=Dominic |title=IC1182 (Galaxy) |url=https://in-the-sky.org//data/object.php?id=IC1182 |access-date=2024-04-30 |website=In-The-Sky.org |language=en}}</ref> It is located 464 million [[Light-year|light-years]] away from the [[Solar System|solar system]]<ref name=":0">{{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=2024-04-30 |website=ned.ipac.caltech.edu}}</ref> and was discovered on August 11, 1892 by [[Stéphane Javelle|Stephane Javelle]].<ref>{{Cite web |title=Index Catalog Objects: IC 1150 - 1199 |url=https://cseligman.com/text/atlas/ic11a.htm#ic1182 |access-date=2024-04-30 |website=cseligman.com}}</ref> IC 1198 is a member of the [[Hercules Cluster]],<ref name=":0" /> which is a part of the [[CfA2 Great Wall|CfA 2 Great Wall]].<ref>{{Cite web |title=Clusters and Superclusters of Galaxies |url=https://ned.ipac.caltech.edu/level5/Sept01/Bahcall2/Bahcall9_2.html |access-date=2024-04-30 |website=ned.ipac.caltech.edu}}</ref>
== Description ==
IC 1182 was originally classified as a [[Seyfert galaxy|Seyfert]] type 2 galaxy but later, research proves, it is indeed an unusual and rare galaxy in some kind of merger event.<ref>{{Cite web |title=Object of the Week May 25, 2014 IC 1182 A Member of The Jet Set |url=https://www.deepskyforum.com/showth...k-May-25-2014-IC-1182-A-Member-of-The-Jet-Set |access-date=2024-04-30 |website=www.deepskyforum.com}}</ref> It presents a [[Astrophysical jet|jet]] that is extending out from the center in east direction comprising of [[Kinetic energy|kinetic material]].<ref name=":1">{{Cite web |last=information@eso.org |title=The VLT Records Faint Structures in Colliding Galaxies |url=https://www.eso.org/public/news/eso9834/ |access-date=2024-04-30 |website=www.eso.org |language=es}}</ref> There is a broad faint S-shaped plume and debris on the other side of the galaxy. Not to mention, IC 1182 radiates a lot of [[energy]] and expels a subsential amount of material at high [[velocity]] into depths of space. In its central region, clusters of [[O-type main-sequence star|O-type]] hot blue stars are present.<ref name=":1" />
== An ongoing merger? ==
IC 1182 shows high resolution broad and narrow band images and long slit [[spectroscopy]]. It reveals a distorted morphology with a heavily [[Interstellar cloud|obscured disk-link structure]] with several knots in its regions.<ref name=":2">{{Cite journal |last=Moles |first=M. |last2=Bettoni |first2=D. |last3=Fasano |first3=G. |last4=Kjærgaard |first4=P. |last5=Varela |first5=J. |last6=Milvang-Jensen |first6=B. |date=2004-05-01 |title=The peculiar galaxy IC 1182: An ongoing merger? |url=https://www.aanda.org/articles/aa/abs/2004/17/aa0295/aa0295.html |journal=Astronomy & Astrophysics |language=en |volume=418 |issue=2 |pages=495–507 |doi=10.1051/0004-6361:20034295 |issn=0004-6361}}</ref> Some of the [[Interstellar medium|galactic material]], in the form of two slender tails are detected beyond the main body of the [[galaxy]]. IC 1182 has [[Color index|color indices]] of an early type object which is significantly bluer than what is typical for the kind of galaxy.<ref name=":2" /> The [[Narrow-line region|narrow lines]] shows this galaxy is a [[Active galactic nucleus|powerful emitter]] which the knots in the central region and inside the tail emerging eastward from the galaxy are [[Luminous efficacy|luminous]] in H''α'' and have typical sizes of 1 kpc.<ref name=":2" />
Additionally, IC 1182 presents large quantities of neural [[hydrogen]] which its distance-independent ratio of hydrogen mass to optical luminosity is equal to 0.7 times the [[Solar radio emission|solar ratio]].<ref name=":3">{{Cite journal |last=Bothun |first=G. D. |last2=Stauffer |first2=J. R. |last3=Schommer |first3=R. A. |date=1981-07-01 |title=The peculiar galaxy IC 1182. |url=https://ui.adsabs.harvard.edu/abs/1981ApJ...247...42B |journal=The Astrophysical Journal |volume=247 |pages=42–47 |doi=10.1086/159007 |issn=0004-637X}}</ref> This might be indicated, it might be in a collision involving a gas-rich spiral which gives rise to observed nuclear [[Spectral line|emission lines]]. <ref name=":3" />
== References ==
<references />
[[Category:IC objects]]
[[Category:UGC objects]]
[[Category:Markarian galaxies]]
[[Category
rincipal Galaxies Catalogue objects]][[Category:Astronomical objects discovered in 1892]]
[[Category:Hercules (constellation)]]
[[Category:LEDA objects]]
[[Category:SDSS objects]]
[[Category:2MASS objects]]
[[Category:Lenticular galaxies]]
[[Category:Hercules Cluster]]
Okumaya devam et...