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	<title>IC 1101 - 版本历史</title>
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	<subtitle>本wiki上该页面的版本历史</subtitle>
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		<title>imported&gt;InternetArchiveBot：​Add 4 books for verifiability (20251017sim)) #IABot (v2.0.9.5) (GreenC bot</title>
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		<summary type="html">&lt;p&gt;Add 4 books for verifiability (20251017sim)) #IABot (v2.0.9.5) (&lt;a href=&quot;/index.php?title=User:GreenC_bot&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;User:GreenC bot（页面不存在）&quot;&gt;GreenC bot&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Infobox galaxy&lt;br /&gt;
| name = [[NGC天體表#IC天體|IC]] 1101&lt;br /&gt;
| image = [[File:Supergalaxia IC 1101.png|400px]]&lt;br /&gt;
| caption = 從左到右依序為[[銀河系]]、[[仙女座星系]]、[[M87]]、&amp;#039;&amp;#039;&amp;#039;IC 1101&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
| epoch = [[J2000.0|J2000]]&lt;br /&gt;
| constellation name = [[室女座]]&lt;br /&gt;
| ra = {{RA|15|10|56.1}}&amp;lt;ref name=&amp;quot;ned&amp;quot;&amp;gt;{{cite web |url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=IC+1101&amp;amp;extend=no&amp;amp;hconst=73&amp;amp;omegam=0.27&amp;amp;omegav=0.73&amp;amp;corr_z=1&amp;amp;out_csys=Equatorial&amp;amp;out_equinox=J2000.0&amp;amp;obj_sort=RA+or+Longitude&amp;amp;of=pre_text&amp;amp;zv_breaker=30000.0&amp;amp;list_limit=5&amp;amp;img_stamp=YES |title=NED results for object IC 1101 |work=NASA/IPAC Extragalactic Database |accessdate=11 November 2006 |archive-date=2019-02-12 |archive-url=https://web.archive.org/web/20190212011626/http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=IC+1101&amp;amp;extend=no&amp;amp;hconst=73&amp;amp;omegam=0.27&amp;amp;omegav=0.73&amp;amp;corr_z=1&amp;amp;out_csys=Equatorial&amp;amp;out_equinox=J2000.0&amp;amp;obj_sort=RA+or+Longitude&amp;amp;of=pre_text&amp;amp;zv_breaker=30000.0&amp;amp;list_limit=5&amp;amp;img_stamp=YES |dead-url=no }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
| dec = {{DEC|+05|44|41}}&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| z = {{val|0.077947|0.000087}}&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| h_radial_v = {{convert|23368|±|26|km/s|abbr=on}}&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| gal_v = {{convert|23395|±|26|km/s|abbr=on}}&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| dist_ly = {{val|10.45|0.73|u=[[光年|億光年]]}} &amp;lt;br/&amp;gt; ({{val|320.5|22.4|u=[[秒差距|Mpc]]}}){{hub|0.73}}&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| group_cluster = [[阿贝尔2029]]&lt;br /&gt;
| type = E/S0&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;/&amp;gt;&lt;br /&gt;
| size = {{val|210|39|u= [[光年|Kly]]}} &amp;lt;br/&amp;gt; （{{val|65|12|u=[[秒差距#秒差距和千秒差距|kpc]]}}）[[有效半徑]]&amp;lt;ref name=&amp;quot;Fisher1995&amp;quot;&amp;gt;{{cite journal |title=Kinematics of 13 brightest cluster galaxies |url=https://archive.org/details/sim_astrophysical-journal_1995-01-10_438_2/page/538 |journal=[[The Astrophysical Journal]] |first1=David |last1=Fisher |first2=Garth |last2=Illingworth |first3=Marijn |last3=Franx |volume=438 |issue=2 |pages=539–562 |date=January 1995 |doi=10.1086/175100 |bibcode=1995ApJ...438..539F}}&amp;lt;/ref&amp;gt;&amp;lt;!-- 42 ± 8 arcsec from Fisher et al 1995, corresponding to 65 ± 12 kpc. 65*3.26 = 201.2, or 210 kly to the uncertainty --&amp;gt;&amp;lt;!--Please see talk page discussion regarding the inaccuracy of 5.5 Mly. This is for the diffuse halo, which is not an accepted measure of galaxy size. The true size is somewhat ambiguous. Therefore, please do NOT either mention the 5.5 Mly size here, or say that this galaxy is the largest known.--&amp;gt;&lt;br /&gt;
| stars = 100 兆 (10&amp;lt;sup&amp;gt;14&amp;lt;/sup&amp;gt;)&amp;lt;!-- exponential value to disambiguate &amp;quot;trillion --&amp;gt;&lt;br /&gt;
| appmag_v = 14.73&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| size_v = 1&amp;#039;.2 × 0&amp;#039;.6&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| notes = &lt;br /&gt;
| names = [[烏普薩拉星系總表|UGC]] 9752,&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt; [[主要星系目錄|PGC]] 54167,&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt; A2029-[[最亮團星系|BCG]]&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;&lt;br /&gt;
| references = &lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;IC 1101&amp;#039;&amp;#039;&amp;#039;是位於[[阿贝尔2029]][[星系團]]中心的一個超巨大[[橢圓星系]]，距離地球大約320[[秒差距|百萬秒差距]]（10.4億[[光年]]）&amp;lt;ref name=&amp;quot;ned&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
== 特性 ==&lt;br /&gt;
這個星系被分類為超巨大橢圓（E）到透鏡狀星系（S0）&amp;lt;ref name=&amp;quot;SIMBAD&amp;quot;&amp;gt;{{cite web |url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=IC+1101 |title=IC 1101 -- Brightest galaxy in a Cluster (BCG) |work=[[SIMBAD]] |accessdate=21 December 2014 |archive-date=2018-09-08 |archive-url=https://web.archive.org/web/20180908063837/http://simbad.u-strasbg.fr/simbad/sim-id?Ident=IC+1101 |dead-url=no }}&amp;lt;/ref&amp;gt;，並且是艾伯耳2029星系團中最亮的星系（它也會被稱為A2029-BCG；BCG的意思是&amp;#039;&amp;#039;[[最亮團星系]]&amp;#039;&amp;#039;）&amp;lt;ref name=&amp;quot;Lewis2003&amp;quot;&amp;gt;{{cite journal |title=&amp;#039;&amp;#039;Chandra&amp;#039;&amp;#039; Observations of A2029: The Dark Matter Profile Down to below 0.01&amp;#039;&amp;#039;r&amp;#039;&amp;#039;&amp;lt;sub&amp;gt;vir&amp;lt;/sub&amp;gt; in an Unusually Relaxed Cluster |url=https://archive.org/details/sim_astrophysical-journal_2003-03-20_586_1/page/134 |journal=[[The Astrophysical Journal]] |first1=Aaron D. |last1=Lewis |first2=David A. |last2=Buote |first3=John T. |last3=Stocke |volume=586 |issue=1 |pages=135–142 |date=March 2003 |doi=10.1086/367556 |bibcode=2003ApJ...586..135L |arxiv=astro-ph/0209205}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;science250_4980_539&amp;quot;&amp;gt;{{cite journal |title=The central galaxy in Abell 2029 - an old supergiant |url=https://archive.org/details/sim_science_1990-10-26_250_4980/page/n83 |journal=[[Science (journal)|Science]] |first1=Juan M. |last1=Uson |first2=Stephen P. |last2=Boughn |first3=Jeffrey R. |last3=Kuhn |volume=250 |issue=4980 |pages=539–540 |date=October 1990 |doi=10.1126/science.250.4980.539 |bibcode=1990Sci...250..539U}}&amp;lt;/ref&amp;gt;。這個星系的型態類型被懷疑是個扁平的圓盤狀，但從地球上看到的只是它最寬廣的一面。然而，多數的透鏡星系的尺寸範圍從15至37[[秒差距|千秒差距]]（5萬至12萬[[光年]]）&amp;lt;ref&amp;gt;{{cite web |url=http://cseligman.com/text/atlas/ngc0a.htm |title=NGC Objects: NGC 50 - 99 |series=Celestial Atlas |work=Cseligman.com |first=Courtney |last=Seligman |accessdate=14 April 2015 |archive-date=2018-10-24 |archive-url=https://web.archive.org/web/20181024090905/http://cseligman.com/text/atlas/ngc0a.htm |dead-url=no }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{specify|note=Where in the source is this stated?|date=January 2016}}&amp;lt;/ref&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
IC 1101是[[巨大星系列表|已知星系中最大]]的，但是如何定義這種星系的大小，在天文學的文獻中仍有爭議。來自星系的藍光[[攝影乾版]]（對恆星的取樣不包括擴散的暈）給予的[[有效半徑]]（輻射出一半光量的半徑）是{{val|65|12|u=kpc}} ({{val|212|39|u=thousand ly}})&amp;lt;ref name=&amp;quot;Fisher1995&amp;quot; /&amp;gt;。這個星系有非常大的低強度&amp;#039;&amp;#039;漫射光&amp;#039;&amp;#039;，半徑延伸至600千秒差距（200萬光年）&amp;lt;ref name=&amp;quot;Uson1991&amp;quot;&amp;gt;{{cite journal |title=Diffuse light in dense clusters of galaxies. I. &amp;#039;&amp;#039;R&amp;#039;&amp;#039;-band observations of Abell 2029 |url=https://archive.org/details/sim_astrophysical-journal_1991-03-01_369_1/page/46 |journal=[[The Astrophysical Journal]] |first1=Juan M. |last1=Uson |first2=Stephen P. |last2=Boughn |first3=Jeffrey R. |last3=Kuhn |volume=369 |pages=46–53 |date=March 1991 |doi=10.1086/169737 |bibcode=1991ApJ...369...46U}}&amp;lt;/ref&amp;gt;。研究IC 1101的作者確認&amp;#039;&amp;#039;若包含暈可能是宇宙中最大和最亮的星系&amp;#039;&amp;#039;&amp;lt;ref name=&amp;quot;Uson1991&amp;quot; /&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
像多數的巨大星系，IC 1101擁有大量的富金屬星，其中有些比太陽老70億歲，因此呈現金黃色的光澤。它在中心有一個與巨大的黑洞，與明亮的無線電源相關聯。&lt;br /&gt;
&lt;br /&gt;
== 發現 ==&lt;br /&gt;
這個星系是在1790年6月19日由英國天文學家[[威廉·赫歇爾]]發現的。它於1895年被[[約翰·路易·埃米爾·德雷耳]]收錄在[[NGC天體表#IC天體|星雲和星團索引目錄]]（IC）中的第1101個天體。當它被發現時，以它的外觀被認為是一個星雲。後來[[愛德溫·哈伯]]在1932年發現一些具有星雲外觀的天體實際上就是獨立的星系，對這些天空中物體進行的後續分析，發現IC 1101是一個獨立的星系。&lt;br /&gt;
&lt;br /&gt;
== 相關條目 ==&lt;br /&gt;
*[[星系列表]]&lt;br /&gt;
*[[星系團]]&lt;br /&gt;
*[[星系團表]]&lt;br /&gt;
*[[星系]]&lt;br /&gt;
&lt;br /&gt;
== 參考資料 ==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
== 外部連結 ==&lt;br /&gt;
* {{cite news |url=http://www.nytimes.com/1990/10/26/us/sighting-of-largest-galaxy-hints-clues-on-the-clustering-of-matter.html |title=Sighting of Largest Galaxy Hints Clues on the Clustering of Matter |work=[[The New York Times]] |first=John Noble |last=Wilford |date=26 October 1990 |accessdate=2016-04-14 |archive-date=2016-03-06 |archive-url=https://web.archive.org/web/20160306164259/http://www.nytimes.com/1990/10/26/us/sighting-of-largest-galaxy-hints-clues-on-the-clustering-of-matter.html |dead-url=no }}&lt;br /&gt;
* {{cite web |url=http://apod.nasa.gov/apod/ap120312.html |title=The Scale of the Universe - Interactive |work=[[Astronomy Picture of the Day]] |date=12 March 2012 |accessdate=2016-04-14 |archive-date=2012-03-14 |archive-url=https://web.archive.org/web/20120314141452/http://apod.nasa.gov/apod/ap120312.html |dead-url=no }}&lt;br /&gt;
* {{WikiSky}}&lt;br /&gt;
&lt;br /&gt;
{{Sky|15|10|56.1|+|05|44|41|1}}&lt;br /&gt;
&lt;br /&gt;
[[Category:橢圓星系]]&lt;br /&gt;
[[Category:室女座]]&lt;br /&gt;
[[Category:IC天體|1101]]&lt;br /&gt;
[[Category:PGC天體|54167]]&lt;br /&gt;
[[Category:UGC天體|09752]]&lt;br /&gt;
[[Category:1790年發現的天體|17900619]]&lt;/div&gt;</summary>
		<author><name>imported&gt;InternetArchiveBot</name></author>
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