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	<id>http://202.127.29.3/~shen/wiki/index.php?action=history&amp;feed=atom&amp;title=BHB_stars</id>
	<title>BHB stars - 版本历史</title>
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	<updated>2026-05-09T14:29:05Z</updated>
	<subtitle>本wiki上该页面的版本历史</subtitle>
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	<entry>
		<id>http://202.127.29.3/~shen/wiki/index.php?title=BHB_stars&amp;diff=1413&amp;oldid=prev</id>
		<title>2014年11月21日 (五) 08:50 Shen</title>
		<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=BHB_stars&amp;diff=1413&amp;oldid=prev"/>
		<updated>2014-11-21T08:50:59Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;←上一版本&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;2014年11月21日 (五) 08:50的版本&lt;/td&gt;
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  &lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;第1行：&lt;/td&gt;
  &lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;第1行：&lt;/td&gt;
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&lt;tr&gt;
  &lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;
  &lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A kind of Population II star, found in the&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;     &lt;/del&gt;  galactic halo and especially in globular&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;      &lt;/del&gt; clusters, that has evolved past the red&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;    &lt;/del&gt;   giant stage and is now burning helium&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;     &lt;/del&gt;  in its core. Blue horizontal-branch (BHB) stars are typically of spectral       type B3 to A0 (hence very blue in color), and have spectra characterized&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;      &lt;/del&gt; by strong, sharp hydrogen lines, a large Balmer&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt; jump (see Balmer       series)&lt;/del&gt;, and very weak lines of other elements. &lt;/div&gt;&lt;/td&gt;
  &lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;
  &lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;A kind of Population II star, found in the  galactic halo and especially in globular clusters, that has evolved past the red   giant stage and is now burning helium  in its core. Blue horizontal-branch (BHB) stars are typically of spectral       type B3 to A0 (hence very blue in color), and have spectra characterized by strong, sharp hydrogen lines, a large Balmer, and very weak lines of other elements. &lt;/div&gt;&lt;/td&gt;
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  &lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;      &lt;/div&gt;&lt;/td&gt;
  &lt;td class=&quot;diff-marker&quot;&gt;&lt;/td&gt;
  &lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;      &lt;/div&gt;&lt;/td&gt;
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  &lt;td class=&quot;diff-marker&quot; data-marker=&quot;−&quot;&gt;&lt;/td&gt;
  &lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;      &lt;/del&gt;BHB stars are found on the horizontal&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;     &lt;/del&gt;  branch of the Hertzsprung-Russell diagram&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;     &lt;/del&gt;  to the left, blue side of RR Lyrae variables.&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;     &lt;/del&gt;  They are very good tracers because of their extreme brightness and the fact&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;     &lt;/del&gt;  that most faint blue stars seen in the halo are usually BHB stars.&lt;/div&gt;&lt;/td&gt;
  &lt;td class=&quot;diff-marker&quot; data-marker=&quot;+&quot;&gt;&lt;/td&gt;
  &lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;BHB stars are found on the horizontal  branch of the Hertzsprung-Russell diagram  to the left, blue side of RR Lyrae variables.  They are very good tracers because of their extreme brightness and the fact  that most faint blue stars seen in the halo are usually BHB stars.&lt;/div&gt;&lt;/td&gt;
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		<author><name>Shen</name></author>
	</entry>
	<entry>
		<id>http://202.127.29.3/~shen/wiki/index.php?title=BHB_stars&amp;diff=1412&amp;oldid=prev</id>
		<title>Shen：​以“A kind of Population II star, found in the       galactic halo and especially in globular       clusters, that has evolved past the red       giant stage and is now ...”为内容创建页面</title>
		<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=BHB_stars&amp;diff=1412&amp;oldid=prev"/>
		<updated>2014-11-21T08:49:43Z</updated>

		<summary type="html">&lt;p&gt;以“A kind of Population II star, found in the       galactic halo and especially in globular       clusters, that has evolved past the red       giant stage and is now ...”为内容创建页面&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;A kind of Population II star, found in the       galactic halo and especially in globular       clusters, that has evolved past the red       giant stage and is now burning helium       in its core. Blue horizontal-branch (BHB) stars are typically of spectral       type B3 to A0 (hence very blue in color), and have spectra characterized       by strong, sharp hydrogen lines, a large Balmer jump (see Balmer       series), and very weak lines of other elements. &lt;br /&gt;
      &lt;br /&gt;
      BHB stars are found on the horizontal       branch of the Hertzsprung-Russell diagram       to the left, blue side of RR Lyrae variables.       They are very good tracers because of their extreme brightness and the fact       that most faint blue stars seen in the halo are usually BHB stars.&lt;/div&gt;</summary>
		<author><name>Shen</name></author>
	</entry>
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