Galaxybeing: Created NGC 5098
{{Infobox galaxy|name=NGC 5098|image=File:NGC 5098 SDSS2.jpg|caption=[[Sloan Digital Sky Survey|SDSS]] image of galaxy pair NGC 5098|constellation name=[[Canes Venatici]]|ra=13h 20m 16.2s|dec=+33d 08m 39s|z=0.037893|h_radial_v=11,360 [[kilometer per second|km/s]]|dist_ly=559 [[Mly]] (171.3 [[Megaparsec|Mpc]])|appmag_v=15.0|group_cluster=NGC 5098 Group|type=S? & S?, E0 & ES-0, E & E|size=128,000 ly (approximately 39.16 [[parsec|kpc]])
& 168,000 ly (approximately 51.60 [[parsec|kpc]])|size_v=0.85 x 0.74 & 0.89 x 0.71|names=[[Principal Galaxies Catalogue|PGC]] 46529 & PGC 46515, [[Morphological Catalogue of Galaxies|MCG]] +06-29-077 & MCG +06-29-78, [[Catalogue of Galaxies and of Clusters of Galaxies|CGCG]] 189-052, B2 1317+33, 7C 1317+3324, [[2MASX]] J13201775+3308409 & 2MASX J13201472+3308359, V1CG 166 NED01 & V1CG NED02, NSA143330 & NSA 091891}}
'''NGC 5098''' are a [[Binary number|binary]] pair of distant [[Galaxy|galaxies]] located in [[Canes Venatici]] constellation.<ref>{{Cite web |title=NGC 5098 - Galaxy Pair in Canes Venatici {{!}} TheSkyLive.com |url=https://theskylive.com/sky/deepsky/ngc5098-object |access-date=2024-05-09 |website=theskylive.com}}</ref><ref>{{Cite web |last=Astronomy |first=Go |title=NGC 5098 {{!}} galaxy pair in Canes Venatici {{!}} NGC List {{!}} GO ASTRONOMY |url=https://www.go-astronomy.com/ngc.php?ID=5438 |access-date=2024-05-09 |website=Go-Astronomy.com |language=en-US}}</ref> They are made up of one Type ES-0<ref name=":0">{{Cite web |title=Revised NGC Data for NGC 5098 |url=http://spider.seds.org/ngc/revngcic.cgi?NGC5098 |access-date=2024-05-09 |website=spider.seds.org}}</ref> [[lenticular galaxy]], '''PGC 46515'''<ref>{{Cite web |title=HyperLeda -object description for PGC 46515 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=PGC 46515 |access-date=2024-05-09 |website=atlas.obs-hp.fr}}</ref> or '''NGC 5098 NED01'''<ref>{{Cite web |title=NED Search Results for NGC 5098 NED01 |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> located [[west]] and one Type E<ref name=":0" /> [[elliptical galaxy]], '''PGC 46529'''<ref>{{Cite web |title=HyperLeda -object description for PGC 46529 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=PGC 46529 |access-date=2024-05-09 |website=atlas.obs-hp.fr}}</ref> or '''NGC 5098 NED02'''<ref>{{Cite web |title=NED Search Results for NGC 5098 NED02 |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> located [[east]]. Both galaxies are located 559 million [[Light-year|light-years]] away from the [[Solar System]]<ref>{{Cite web |title=NED Search Results for NGC 5098 |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> and were discovered on April 29, 1827, by [[John Herschel]].<ref>{{Cite web |title=New General Catalog Objects: NGC 5050 - 5099 |url=https://cseligman.com/text/atlas/ngc50a.htm#5098 |access-date=2024-05-09 |website=cseligman.com}}</ref>
== Characteristics ==
NGC 5098 belongs to the NGC 5098 [[galaxy group]] which is located some 560 million [[Light-year|light-years]] away.<ref>{{Cite web |title=NED Search Results for NGC 5098 GROUP |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> They are the central galaxy pair, first identified by Ramella et al. 1995 "their group 80."<ref>{{Cite journal |last=Ramella |first=Massimo |last2=Geller |first2=Margaret J. |last3=Huchra |first3=John P. |last4=Thorstensen |first4=John R. |date=1995-04-01 |title=The Redshift-Space Neighborhoods of 36 Loose Groups of Galaxies.I.The Data |url=https://ui.adsabs.harvard.edu/abs/1995AJ....109.1458R |journal=The Astronomical Journal |volume=109 |pages=1458 |doi=10.1086/117375 |issn=0004-6256}}</ref> NGC 5098 NED01 is the brighter and larger of the two, showing [[Apparent magnitude|optical magnitudes]] of ''MB'' = −21.131 and ''MV'' = −22.097, as compared to ''MB'' = −20.845 and ''MV'' = −21.770 for NGC 5098 NED02, which the [[Magnitude (astronomy)|magnitudes]] were calculated from [[Sloan Digital Sky Survey]] by Adelman-McCarthy<ref>{{Cite journal |last=Adelman‐McCarthy |first=Jennifer K. |last2=Agüeros |first2=Marcel A. |last3=Allam |first3=Sahar S. |last4=Allende Prieto |first4=Carlos |last5=Anderson |first5=Kurt S.J. |last6=Anderson |first6=Scott F. |last7=Annis |first7=James |last8=Bahcall |first8=Neta A. |last9=Bailer‐Jones |first9=C. A. L. |last10=Baldry |first10=Ivan K. |last11=Barentine |first11=J. C. |last12=Bassett |first12=Bruce A. |last13=Becker |first13=Andrew C. |last14=Beers |first14=Timothy C. |last15=Bell |first15=Eric F. |date=2008-04 |title=The Sixth Data Release of the Sloan Digital Sky Survey |url=https://iopscience.iop.org/article/10.1086/524984 |journal=The Astrophysical Journal Supplement Series |volume=175 |issue=2 |pages=297–313 |doi=10.1086/524984 |issn=0067-0049}}</ref> and converted to Johnson filter system via the relations provided by Smith et al.<ref>{{Cite journal |last=Smith |first=J. Allyn |last2=Tucker |first2=Douglas L. |last3=Kent |first3=Stephen |last4=Richmond |first4=Michael W. |last5=Fukugita |first5=Masataka |last6=Ichikawa |first6=Takashi |last7=Ichikawa |first7=Shin-ichi |last8=Jorgensen |first8=Anders M. |last9=Uomoto |first9=Alan |last10=Gunn |first10=James E. |last11=Hamabe |first11=Masaru |last12=Watanabe |first12=Masaru |last13=Tolea |first13=Alin |last14=Henden |first14=Arne |last15=Annis |first15=James |date=2002-04 |title=The ugriz Standard-Star System |url=https://iopscience.iop.org/article/10.1086/339311 |journal=The Astronomical Journal |volume=123 |issue=4 |pages=2121–2144 |doi=10.1086/339311 |issn=0004-6256}}</ref>
NGC 5098 NED01 hosts an extended [[Astronomical radio source|radio source]], B2 1317+33 which was detected at several [[Frequency|frequencies]].<ref>{{Cite journal |last=Colla |first=G. |last2=Fanti |first2=C. |last3=Ficarra |first3=A. |last4=Formiggini |first4=L. |last5=Gandolfi |first5=E. |last6=Grueff |first6=G. |last7=Lari |first7=C. |last8=Padrielli |first8=L. |last9=Roffi |first9=G. |last10=Tomasi |first10=P. |last11=Vigotti |first11=M. |date=1970-03-01 |title=A catalogue of 3235 radio sources at 408 MHz |url=https://ui.adsabs.harvard.edu/abs/1970A&AS....1..281C |journal=Astronomy and Astrophysics Supplement Series |volume=1 |pages=281 |issn=0365-0138}}</ref> A study showed there is evidence of gas swooshing and [[active galactic nucleus]] (AGN) heating up which the most likely contributor is the nearby galaxy, NGC 5098 NED02 which is being stripped of its gaseous [[atmosphere]].<ref name=":1">{{Cite journal |last=Randall |first=S. W. |last2=Jones |first2=C. |last3=Markevitch |first3=M. |last4=Blanton |first4=E. L. |last5=Nulsen |first5=P. E. J. |last6=Forman |first6=W. R. |date=2009-07-14 |title=GAS SLOSHING AND BUBBLES IN THE GALAXY GROUP NGC 5098 |url=https://iopscience.iop.org/article/10.1088/0004-637X/700/2/1404 |journal=The Astrophysical Journal |volume=700 |issue=2 |pages=1404–1414 |doi=10.1088/0004-637x/700/2/1404 |issn=0004-637X}}</ref> Significant [[cavities]] are present in the central region, which two distinctive bubbles are located north and northeast. They are similar to X-ray [[Observation|observations]] of other galaxies, groups and [[Clusters of galaxies|clusters]].<ref name=":1" /> These are formed when active galactic nucleus (AGN) jets push into local ICM, evacuating cavities and creating bright rims of X-ray emission from displaced gas.<ref name=":1" />
A plume of [[Emission spectrum|emission]] is seen extending northeast from NGC 5098 NED01,<ref>{{Cite journal |last=Gastaldello |first=Fabio |last2=Buote |first2=David A. |last3=Humphrey |first3=Philip J. |last4=Zappacosta |first4=Luca |last5=Bullock |first5=James S. |last6=Brighenti |first6=Fabrizio |last7=Mathews |first7=William G. |date=2007-11 |title=Probing the Dark Matter and Gas Fraction in Relaxed Galaxy Groups with X‐Ray Observations from<i>Chandra</i>and<i>XMM‐Newton</i> |url=https://iopscience.iop.org/article/10.1086/521519 |journal=The Astrophysical Journal |volume=669 |issue=1 |pages=158–183 |doi=10.1086/521519 |issn=0004-637X}}</ref> exhibiting a [[spiral arm]] morphology which originates east from the galaxy and wrapping around to the [[north]]. This presence of a feature indicates NGC 5098 NED01 is indeed [[Interacting galaxy|interacting]] with NGC NED02.<ref name=":1" />
Apart from that, there is a sharp [[surface brightness]] to west, southwest and south, which is approximately 28 kpc from the central AGN of NGC 5098 NED01.<ref name=":1" /> It appears to go eastwards and define the outer [[boundaries]] of the arm, adding to the overall impression of the spiral pattern in diffuse emission. The edges are quite similar to features that are seen from cold fronts generated by [[gas]] sloshing in observations<ref>{{Cite journal |last=Dupke |first=Renato |last2=White III |first2=Raymond E. |last3=Bregman |first3=Joel N. |date=2007-12-10 |title=Different Methods of Forming Cold Fronts in Nonmerging Clusters |url=https://iopscience.iop.org/article/10.1086/522194 |journal=The Astrophysical Journal |volume=671 |issue=1 |pages=181–189 |doi=10.1086/522194 |issn=0004-637X}}</ref> and [[Simulation|stimulations]] of galaxy clusters and groups.<ref name=":2">{{Cite journal |last=Ascasibar |first=Yago |last2=Markevitch |first2=Maxim |date=2006-10-10 |title=The Origin of Cold Fronts in the Cores of Relaxed Galaxy Clusters |url=https://iopscience.iop.org/article/10.1086/506508 |journal=The Astrophysical Journal |volume=650 |issue=1 |pages=102–127 |doi=10.1086/506508 |issn=0004-637X}}</ref>
A study shows NGC 5098 NED02, does not show any traces of associate emission in [[X-ray|X-rays]], implying it was stripped of gas.<ref name=":1" /> It is possible NGC 5098 NED02 after being [[Ram pressure|ram-pressured]] stripped and passing east of NGC 5098 NED01 might have circled around it and now moving east, creating a conical wake in diffuse emission.<ref name=":2" />
== References ==
<references />
[[Category:NGC objects]]
[[Category
iscoveries by John Herschel]]
[[Category:Canes Venatici]]
[[Category:Lenticular galaxies]]
[[Category:Elliptical galaxies]]
[[Category:2MASS objects]]
[[Category:Astronomical objects discovered in 1827]]
[[Categoryrincipal Galaxies Catalogue objects]]
[[Category:MCG objects]]
Okumaya devam et...
{{Infobox galaxy|name=NGC 5098|image=File:NGC 5098 SDSS2.jpg|caption=[[Sloan Digital Sky Survey|SDSS]] image of galaxy pair NGC 5098|constellation name=[[Canes Venatici]]|ra=13h 20m 16.2s|dec=+33d 08m 39s|z=0.037893|h_radial_v=11,360 [[kilometer per second|km/s]]|dist_ly=559 [[Mly]] (171.3 [[Megaparsec|Mpc]])|appmag_v=15.0|group_cluster=NGC 5098 Group|type=S? & S?, E0 & ES-0, E & E|size=128,000 ly (approximately 39.16 [[parsec|kpc]])
& 168,000 ly (approximately 51.60 [[parsec|kpc]])|size_v=0.85 x 0.74 & 0.89 x 0.71|names=[[Principal Galaxies Catalogue|PGC]] 46529 & PGC 46515, [[Morphological Catalogue of Galaxies|MCG]] +06-29-077 & MCG +06-29-78, [[Catalogue of Galaxies and of Clusters of Galaxies|CGCG]] 189-052, B2 1317+33, 7C 1317+3324, [[2MASX]] J13201775+3308409 & 2MASX J13201472+3308359, V1CG 166 NED01 & V1CG NED02, NSA143330 & NSA 091891}}
'''NGC 5098''' are a [[Binary number|binary]] pair of distant [[Galaxy|galaxies]] located in [[Canes Venatici]] constellation.<ref>{{Cite web |title=NGC 5098 - Galaxy Pair in Canes Venatici {{!}} TheSkyLive.com |url=https://theskylive.com/sky/deepsky/ngc5098-object |access-date=2024-05-09 |website=theskylive.com}}</ref><ref>{{Cite web |last=Astronomy |first=Go |title=NGC 5098 {{!}} galaxy pair in Canes Venatici {{!}} NGC List {{!}} GO ASTRONOMY |url=https://www.go-astronomy.com/ngc.php?ID=5438 |access-date=2024-05-09 |website=Go-Astronomy.com |language=en-US}}</ref> They are made up of one Type ES-0<ref name=":0">{{Cite web |title=Revised NGC Data for NGC 5098 |url=http://spider.seds.org/ngc/revngcic.cgi?NGC5098 |access-date=2024-05-09 |website=spider.seds.org}}</ref> [[lenticular galaxy]], '''PGC 46515'''<ref>{{Cite web |title=HyperLeda -object description for PGC 46515 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=PGC 46515 |access-date=2024-05-09 |website=atlas.obs-hp.fr}}</ref> or '''NGC 5098 NED01'''<ref>{{Cite web |title=NED Search Results for NGC 5098 NED01 |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> located [[west]] and one Type E<ref name=":0" /> [[elliptical galaxy]], '''PGC 46529'''<ref>{{Cite web |title=HyperLeda -object description for PGC 46529 |url=http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=PGC 46529 |access-date=2024-05-09 |website=atlas.obs-hp.fr}}</ref> or '''NGC 5098 NED02'''<ref>{{Cite web |title=NED Search Results for NGC 5098 NED02 |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> located [[east]]. Both galaxies are located 559 million [[Light-year|light-years]] away from the [[Solar System]]<ref>{{Cite web |title=NED Search Results for NGC 5098 |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> and were discovered on April 29, 1827, by [[John Herschel]].<ref>{{Cite web |title=New General Catalog Objects: NGC 5050 - 5099 |url=https://cseligman.com/text/atlas/ngc50a.htm#5098 |access-date=2024-05-09 |website=cseligman.com}}</ref>
== Characteristics ==
NGC 5098 belongs to the NGC 5098 [[galaxy group]] which is located some 560 million [[Light-year|light-years]] away.<ref>{{Cite web |title=NED Search Results for NGC 5098 GROUP |url=https://ned.ipac.caltech.edu/cgi-bi...&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1 |access-date=2024-05-09 |website=ned.ipac.caltech.edu}}</ref> They are the central galaxy pair, first identified by Ramella et al. 1995 "their group 80."<ref>{{Cite journal |last=Ramella |first=Massimo |last2=Geller |first2=Margaret J. |last3=Huchra |first3=John P. |last4=Thorstensen |first4=John R. |date=1995-04-01 |title=The Redshift-Space Neighborhoods of 36 Loose Groups of Galaxies.I.The Data |url=https://ui.adsabs.harvard.edu/abs/1995AJ....109.1458R |journal=The Astronomical Journal |volume=109 |pages=1458 |doi=10.1086/117375 |issn=0004-6256}}</ref> NGC 5098 NED01 is the brighter and larger of the two, showing [[Apparent magnitude|optical magnitudes]] of ''MB'' = −21.131 and ''MV'' = −22.097, as compared to ''MB'' = −20.845 and ''MV'' = −21.770 for NGC 5098 NED02, which the [[Magnitude (astronomy)|magnitudes]] were calculated from [[Sloan Digital Sky Survey]] by Adelman-McCarthy<ref>{{Cite journal |last=Adelman‐McCarthy |first=Jennifer K. |last2=Agüeros |first2=Marcel A. |last3=Allam |first3=Sahar S. |last4=Allende Prieto |first4=Carlos |last5=Anderson |first5=Kurt S.J. |last6=Anderson |first6=Scott F. |last7=Annis |first7=James |last8=Bahcall |first8=Neta A. |last9=Bailer‐Jones |first9=C. A. L. |last10=Baldry |first10=Ivan K. |last11=Barentine |first11=J. C. |last12=Bassett |first12=Bruce A. |last13=Becker |first13=Andrew C. |last14=Beers |first14=Timothy C. |last15=Bell |first15=Eric F. |date=2008-04 |title=The Sixth Data Release of the Sloan Digital Sky Survey |url=https://iopscience.iop.org/article/10.1086/524984 |journal=The Astrophysical Journal Supplement Series |volume=175 |issue=2 |pages=297–313 |doi=10.1086/524984 |issn=0067-0049}}</ref> and converted to Johnson filter system via the relations provided by Smith et al.<ref>{{Cite journal |last=Smith |first=J. Allyn |last2=Tucker |first2=Douglas L. |last3=Kent |first3=Stephen |last4=Richmond |first4=Michael W. |last5=Fukugita |first5=Masataka |last6=Ichikawa |first6=Takashi |last7=Ichikawa |first7=Shin-ichi |last8=Jorgensen |first8=Anders M. |last9=Uomoto |first9=Alan |last10=Gunn |first10=James E. |last11=Hamabe |first11=Masaru |last12=Watanabe |first12=Masaru |last13=Tolea |first13=Alin |last14=Henden |first14=Arne |last15=Annis |first15=James |date=2002-04 |title=The ugriz Standard-Star System |url=https://iopscience.iop.org/article/10.1086/339311 |journal=The Astronomical Journal |volume=123 |issue=4 |pages=2121–2144 |doi=10.1086/339311 |issn=0004-6256}}</ref>
NGC 5098 NED01 hosts an extended [[Astronomical radio source|radio source]], B2 1317+33 which was detected at several [[Frequency|frequencies]].<ref>{{Cite journal |last=Colla |first=G. |last2=Fanti |first2=C. |last3=Ficarra |first3=A. |last4=Formiggini |first4=L. |last5=Gandolfi |first5=E. |last6=Grueff |first6=G. |last7=Lari |first7=C. |last8=Padrielli |first8=L. |last9=Roffi |first9=G. |last10=Tomasi |first10=P. |last11=Vigotti |first11=M. |date=1970-03-01 |title=A catalogue of 3235 radio sources at 408 MHz |url=https://ui.adsabs.harvard.edu/abs/1970A&AS....1..281C |journal=Astronomy and Astrophysics Supplement Series |volume=1 |pages=281 |issn=0365-0138}}</ref> A study showed there is evidence of gas swooshing and [[active galactic nucleus]] (AGN) heating up which the most likely contributor is the nearby galaxy, NGC 5098 NED02 which is being stripped of its gaseous [[atmosphere]].<ref name=":1">{{Cite journal |last=Randall |first=S. W. |last2=Jones |first2=C. |last3=Markevitch |first3=M. |last4=Blanton |first4=E. L. |last5=Nulsen |first5=P. E. J. |last6=Forman |first6=W. R. |date=2009-07-14 |title=GAS SLOSHING AND BUBBLES IN THE GALAXY GROUP NGC 5098 |url=https://iopscience.iop.org/article/10.1088/0004-637X/700/2/1404 |journal=The Astrophysical Journal |volume=700 |issue=2 |pages=1404–1414 |doi=10.1088/0004-637x/700/2/1404 |issn=0004-637X}}</ref> Significant [[cavities]] are present in the central region, which two distinctive bubbles are located north and northeast. They are similar to X-ray [[Observation|observations]] of other galaxies, groups and [[Clusters of galaxies|clusters]].<ref name=":1" /> These are formed when active galactic nucleus (AGN) jets push into local ICM, evacuating cavities and creating bright rims of X-ray emission from displaced gas.<ref name=":1" />
A plume of [[Emission spectrum|emission]] is seen extending northeast from NGC 5098 NED01,<ref>{{Cite journal |last=Gastaldello |first=Fabio |last2=Buote |first2=David A. |last3=Humphrey |first3=Philip J. |last4=Zappacosta |first4=Luca |last5=Bullock |first5=James S. |last6=Brighenti |first6=Fabrizio |last7=Mathews |first7=William G. |date=2007-11 |title=Probing the Dark Matter and Gas Fraction in Relaxed Galaxy Groups with X‐Ray Observations from<i>Chandra</i>and<i>XMM‐Newton</i> |url=https://iopscience.iop.org/article/10.1086/521519 |journal=The Astrophysical Journal |volume=669 |issue=1 |pages=158–183 |doi=10.1086/521519 |issn=0004-637X}}</ref> exhibiting a [[spiral arm]] morphology which originates east from the galaxy and wrapping around to the [[north]]. This presence of a feature indicates NGC 5098 NED01 is indeed [[Interacting galaxy|interacting]] with NGC NED02.<ref name=":1" />
Apart from that, there is a sharp [[surface brightness]] to west, southwest and south, which is approximately 28 kpc from the central AGN of NGC 5098 NED01.<ref name=":1" /> It appears to go eastwards and define the outer [[boundaries]] of the arm, adding to the overall impression of the spiral pattern in diffuse emission. The edges are quite similar to features that are seen from cold fronts generated by [[gas]] sloshing in observations<ref>{{Cite journal |last=Dupke |first=Renato |last2=White III |first2=Raymond E. |last3=Bregman |first3=Joel N. |date=2007-12-10 |title=Different Methods of Forming Cold Fronts in Nonmerging Clusters |url=https://iopscience.iop.org/article/10.1086/522194 |journal=The Astrophysical Journal |volume=671 |issue=1 |pages=181–189 |doi=10.1086/522194 |issn=0004-637X}}</ref> and [[Simulation|stimulations]] of galaxy clusters and groups.<ref name=":2">{{Cite journal |last=Ascasibar |first=Yago |last2=Markevitch |first2=Maxim |date=2006-10-10 |title=The Origin of Cold Fronts in the Cores of Relaxed Galaxy Clusters |url=https://iopscience.iop.org/article/10.1086/506508 |journal=The Astrophysical Journal |volume=650 |issue=1 |pages=102–127 |doi=10.1086/506508 |issn=0004-637X}}</ref>
A study shows NGC 5098 NED02, does not show any traces of associate emission in [[X-ray|X-rays]], implying it was stripped of gas.<ref name=":1" /> It is possible NGC 5098 NED02 after being [[Ram pressure|ram-pressured]] stripped and passing east of NGC 5098 NED01 might have circled around it and now moving east, creating a conical wake in diffuse emission.<ref name=":2" />
== References ==
<references />
[[Category:NGC objects]]
[[Category
iscoveries by John Herschel]][[Category:Canes Venatici]]
[[Category:Lenticular galaxies]]
[[Category:Elliptical galaxies]]
[[Category:2MASS objects]]
[[Category:Astronomical objects discovered in 1827]]
[[Category
rincipal Galaxies Catalogue objects]][[Category:MCG objects]]
Okumaya devam et...