https://arolstar52-zhtest.hf.space/index.php?action=history&feed=atom&title=NGC_3191
NGC 3191 - 版本历史
2026-07-18T19:38:22Z
本wiki上该页面的版本历史
MediaWiki 1.43.9
https://arolstar52-zhtest.hf.space/index.php?title=NGC_3191&diff=4016883&oldid=prev
imported>InternetArchiveBot：补救3个来源，并将0个来源标记为失效。) #IABot (v2.0.8.9
2022-08-08T03:32:31Z
<p>补救3个来源，并将0个来源标记为失效。) #IABot (v2.0.8.9</p>
<p><b>新页面</b></p><div>{{Infobox galaxy<br />
| name = [[NGC天體表|NGC]] 3191<br />
| image = File:NGC3191 - SDSS DR14.jpg<br />
| caption = [[史隆數位巡天|SDSS]]拍摄的NGC 3191（中）<br />
| credit =<br />
| epoch = [[曆元|J2000]]<br />
| type = SB(s)bc pec <ref name="ned">{{cite web<br />
| title=NASA/IPAC Extragalactic Database<br />
| work=Results for NGC 3191<br />
| url=http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+3191<br />
| accessdate=2016-01-18<br />
| archive-date=2019-12-07<br />
| archive-url=https://web.archive.org/web/20191207170645/http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+3191<br />
| dead-url=no<br />
}}</ref><br />
| ra = {{RA|10|19|05.1}}<ref name="ned" /> <br />
| dec = {{DEC|46|27|15}}<ref name="ned" /><br />
| dist_ly = [[数量级 (长度)|411]] [[光年|Mly]] (126 [[秒差距|Mpc]])<ref name="ned" /><br />
| z = 9182 ± 4 [[公里|km]]/[[秒|s]]<ref name="ned" /><br />
| appmag_v = 13.2<br />
| size_v = 0&prime;.8 × 0&prime;.6<ref name="ned" /><br />
| constellation name = [[大熊座]]<br />
| notes = <br />
| names = NGC 3192, [[乌普萨拉总目录|UGC]] 5565, [[星系形态目录|MCG]] +08-19-018, [[主要星系目录|PGC]] 30136<ref name="ned" /><br />
}}<br />
'''NGC 3191'''（又名'''NGC 3192'''）是一个位于[[大熊座]]的[[棒旋星系]]，距离地球4亿[[光年]]，直径11.5万光年。NGC 3191与其西边1.3弧分的星系形成[[交互作用星系]]，两星系间形成蓝色的潮汐桥<ref>{{cite journal|last1=Takeuchi|first1=Tsutomu T.|last2=Tomita|first2=Akihiko|last3=Nakanishi|first3=Kouichiro|last4=Ishii|first4=Takako T.|last5=Iwata|first5=Ikuru|last6=Saito|first6=Mamoru|title=Photometric Properties of Kiso Ultraviolet - Excess Galaxies in the Lynx - Ursa Major Region|journal=The Astrophysical Journal Supplement Series|date=April 1999|volume=121|issue=2|pages=445–472|doi=10.1086/313203|arxiv = astro-ph/9810161 |bibcode = 1999ApJS..121..445T |s2cid=15506322}}</ref>。研究人员在NGC 3191中发现了[[超新星]]'''SN 1988B'''和'''SN 2017egm'''。SN 1988B出现在星系中心偏北10[[角秒]]处。SN 2017egm在2017年5月23日由[[盖亚任务]]发现，是一颗[[Ia型超新星]]<ref>{{cite web|title=IAUC 4533|url=http://www.cbat.eps.harvard.edu/iauc/04500/04533.html|publisher=Central Bureau for Astronomical Telegrams|accessdate=29 June 2017|archive-date=2017-08-02|archive-url=https://web.archive.org/web/20170802135535/http://www.cbat.eps.harvard.edu/iauc/04500/04533.html|dead-url=no}}</ref><ref>{{cite web|title=IAUC 4535|url=http://www.cbat.eps.harvard.edu/iauc/04500/04535.html|publisher=Central Bureau for Astronomical Telegrams|accessdate=29 June 2017|archive-date=2017-08-02|archive-url=https://web.archive.org/web/20170802133558/http://www.cbat.eps.harvard.edu/iauc/04500/04535.html|dead-url=no}}</ref><ref>{{cite journal|last1=Bose|first1=Subhash|last2=Dong|first2=Subo|last3=Pastorello|first3=A.|last4=Filippenko|first4=Alexei V.|last5=Kochanek|first5=C. S.|last6=Mauerhan|first6=Jon|last7=Romero-Canizales|first7=C.|last8=Brink|first8=Thomas|last9=Chen|first9=Ping|last10=Prieto|first10=J. L.|last11=Post|first11=R.|last12=Ashall|first12=Christopher|last13=Grupe|first13=Dirk|last14=Tomasella|first14=L.|last15=Benetti|first15=Stefano|last16=Shappee|first16=B. J.|last17=Stanek|first17=K. Z.|last18=Cai|first18=Zheng|last19=Falco|first19=E.|last20=Lundqvist|first20=Peter|last21=Mattila|first21=Seppo|last22=Mutel|first22=Robert|last23=Ochner|first23=Paolo|last24=Pooley|first24=David|last25=Stritzinger|first25=M. D.|last26=Villanueva Jr.|first26=S.|last27=Zheng|first27=WeiKang|last28=Beswick|first28=R. J.|last29=Brown|first29=Peter J.|last30=Cappellaro|first30=E.|last31=Davis|first31=Scott|last32=Fraser|first32=Morgan|last33=de Jaeger|first33=Thomas|last34=Elias-Rosa|first34=N.|last35=Gall|first35=C.|last36=Gaudi|first36=B. Scott|last37=Herczeg|first37=Gregory J.|last38=Hestenes|first38=Julia|last39=Holoien|first39=T. W.-S.|last40=Hosseinzadeh|first40=Griffin|last41=Hsiao|first41=E. Y.|last42=Hu|first42=Shaoming|last43=Jaejin|first43=Shin|last44=Jeffers|first44=Ben|last45=Koff|first45=R. A.|last46=Kumar|first46=Sahana|last47=Kurtenkov|first47=Alexander|last48=Lau|first48=Marie Wingyee|last49=Prentice|first49=Simon|last50=Reynolds|first50=T.|last51=Rudy|first51=Richard J.|last52=Shahbandeh|first52=Melissa|last53=Somero|first53=Auni|last54=Stassun|first54=Keivan G.|last55=Thompson|first55=T. A.|last56=Valenti|first56=Stefano|last57=Woo|first57=Jong-Hak|last58=Yunus|first58=Sameen|title=Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy|journal=The Astrophysical Journal|date=2 August 2017|volume=853|issue=1|pages=57|doi=10.3847/1538-4357/aaa298|bibcode = 2018ApJ...853...57B |arxiv=1708.00864|s2cid=54610579|issn=1538-4357| display-authors = 6}}</ref>。<br />
<br />
== 参考 ==<br />
{{reflist}}<br />
<br />
== 外部链接 ==<br />
*{{commonscat-inline}}<br />
{{wikiSky}}<br />
<br />
<br />
{{Ngc35}}<br />
<br />
[[Category:棒旋星系]]<br />
[[Category:大熊座]]<br />
[[Category:NGC天体|3191]]<br />
[[Category:UGC天體|05565]]<br />
[[Category:PGC天體|30136]]</div>
imported>InternetArchiveBot