<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="zh-Hans-CN">
	<id>http://202.127.29.3/~shen/wiki/index.php?action=history&amp;feed=atom&amp;title=%E5%8F%8C%E6%98%9F</id>
	<title>双星 - 版本历史</title>
	<link rel="self" type="application/atom+xml" href="http://202.127.29.3/~shen/wiki/index.php?action=history&amp;feed=atom&amp;title=%E5%8F%8C%E6%98%9F"/>
	<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=%E5%8F%8C%E6%98%9F&amp;action=history"/>
	<updated>2026-05-25T21:15:50Z</updated>
	<subtitle>本wiki上该页面的版本历史</subtitle>
	<generator>MediaWiki 1.38.1</generator>
	<entry>
		<id>http://202.127.29.3/~shen/wiki/index.php?title=%E5%8F%8C%E6%98%9F&amp;diff=4136&amp;oldid=prev</id>
		<title>Shen：​创建页面，内容为“ *cogsworth[https://arxiv.org/pdf/2409.04543]: is a code that combines binary population synthesis simulations (via COSMIC, Breivik et al. 2020a) with galactic dynamics (via Gala, Price-Whelan 2017) to self-consistently use stellar and orbital evolution to rapidly derive present day positions, kinematics and de�mographics for complete populations of binary stars and their descendants.”</title>
		<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=%E5%8F%8C%E6%98%9F&amp;diff=4136&amp;oldid=prev"/>
		<updated>2024-09-10T13:51:28Z</updated>

		<summary type="html">&lt;p&gt;创建页面，内容为“ *cogsworth[https://arxiv.org/pdf/2409.04543]: is a code that combines binary population synthesis simulations (via &lt;a href=&quot;/~shen/wiki/index.php?title=COSMIC&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;COSMIC（页面不存在）&quot;&gt;COSMIC&lt;/a&gt;, Breivik et al. 2020a) with galactic dynamics (via &lt;a href=&quot;/~shen/wiki/index.php?title=Gala&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;Gala（页面不存在）&quot;&gt;Gala&lt;/a&gt;, Price-Whelan 2017) to self-consistently use stellar and orbital evolution to rapidly derive present day positions, kinematics and de�mographics for complete populations of binary stars and their descendants.”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&lt;br /&gt;
*cogsworth[https://arxiv.org/pdf/2409.04543]: is a code that combines binary population synthesis simulations (via [[COSMIC]], Breivik et al. 2020a) with galactic dynamics (via [[Gala]], Price-Whelan 2017) to self-consistently use stellar and orbital evolution to rapidly derive present day positions, kinematics and de�mographics for complete populations of binary stars and their descendants.&lt;/div&gt;</summary>
		<author><name>Shen</name></author>
	</entry>
</feed>