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	<id>https://arolstar52-zhtest.hf.space/index.php?action=history&amp;feed=atom&amp;title=MWC_480</id>
	<title>MWC 480 - 版本历史</title>
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	<updated>2026-07-18T16:09:40Z</updated>
	<subtitle>本wiki上该页面的版本历史</subtitle>
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	<entry>
		<id>https://arolstar52-zhtest.hf.space/index.php?title=MWC_480&amp;diff=2615040&amp;oldid=prev</id>
		<title>2023年3月22日 (三) 11:35 imported&gt;Phyblas</title>
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		<updated>2023-03-22T11:35:14Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[[File:Artist impression of the protoplanetary disc surrounding the young star MWC 480.webm|thumb|藝術家想像在MWC 480周圍的原行星盤。]]&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;MWC 480&amp;#039;&amp;#039;&amp;#039;是一顆年輕的恆星，距離大約455光年，質量大約是太陽的兩倍，位置在[[金牛座]]的恆星形成區&amp;lt;ref&amp;gt;{{cite web |url=http://arxiv.org/pdf/0911.5457v2 |format=PDF |title=The Disk Population of the Taurus Star-Forming Region |author=K. L. Luhman |display-authors=etal |publisher=Arxiv.org |accessdate=2015-04-08 |archive-date=2019-10-18 |archive-url=https://web.archive.org/web/20191018095703/https://arxiv.org/pdf/0911.5457v2.pdf |dead-url=no }}&amp;lt;/ref&amp;gt;。它的名稱是源自威爾遜山有明亮氫譜線的A和B型恆星目錄（Mount Wilson Catalog of B and A stars with bright hydrogen lines in their spectra）&amp;lt;ref&amp;gt;{{cite web |url=http://www.circumstellardisks.org/show.php?id=101 |title=Catalog of Resolved Circumstellar Disks |work=Circumstellardisks.org |accessdate=2015-04-08 |deadurl=yes |archiveurl=https://web.archive.org/web/20150205014851/http://circumstellardisks.org/show.php?id=101 |archivedate=2015-02-05 }}&amp;lt;/ref&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
MWC 480 是有著X射線輻射的典型前主序[[赫比格Ae/Be星]]，但光電吸收多了一個數量級&amp;lt;ref&amp;gt;{{cite web|url=http://iopscience.iop.org/0004-637X/719/2/1565|title=LOCATING THE ACCRETION FOOTPRINT ON A HERBIG Ae STAR: MWC 480|author=|work=IOP.org |accessdate=2015-04-08}}&amp;lt;/ref&amp;gt;。它有一個被原行星盤環繞的氣體殼層。天文學家使用ALMA（阿塔卡馬大型毫米及次毫米波陣列）已經發現環繞著MWC 480的原行星盤含有大量的複雜碳基分子[[乙腈]]（CH&amp;lt;sub&amp;gt;3&amp;lt;/sub&amp;gt;CN）&amp;lt;ref&amp;gt;{{cite web|url=http://www.eso.org/public/news/eso1513/|title=Complex Organic Molecules Discovered in Infant Star System|author=|work=Eso.org|accessdate=2015-04-08|archive-date=2020-11-08|archive-url=https://web.archive.org/web/20201108174118/https://www.eso.org/public/news/eso1513/|dead-url=no}}&amp;lt;/ref&amp;gt;，在盤中也發現了氰化氫（HCN）&amp;lt;ref&amp;gt;{{cite web|url=http://www.science20.com/news_articles/complex_organic_molecules_discovered_around_star_mwc_480-154667|title=Complex Organic Molecules Discovered Around Star MWC 480|work=Science 2.0|accessdate=2015-04-08|archive-date=2016-03-04|archive-url=https://web.archive.org/web/20160304102710/http://www.science20.com/news_articles/complex_organic_molecules_discovered_around_star_mwc_480-154667|dead-url=no}}&amp;lt;/ref&amp;gt;；但尚未見檢測到行星形成的跡象。&lt;br /&gt;
&lt;br /&gt;
== 參考資料 ==&lt;br /&gt;
[[File:The sky around the young star MWC 480.jpg|thumb|right|年輕恆星MWC 480與周圍的星空。]]&lt;br /&gt;
 &lt;br /&gt;
 {{Reflist}}&lt;br /&gt;
&lt;br /&gt;
[[Category:金牛座]]&lt;br /&gt;
[[Category:恆星]]&lt;/div&gt;</summary>
		<author><name>imported&gt;Phyblas</name></author>
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