<?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=K-Z_relation</id>
	<title>K-Z relation - 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=K-Z_relation"/>
	<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=K-Z_relation&amp;action=history"/>
	<updated>2026-05-13T07:39:30Z</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=K-Z_relation&amp;diff=1933&amp;oldid=prev</id>
		<title>Shen：​创建页面，内容为“The K-z relation for radio galaxies *a tight relationship between their near-infrared K-band magnitudes and their radio luminosities *host galaxies of powerful radio...”</title>
		<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=K-Z_relation&amp;diff=1933&amp;oldid=prev"/>
		<updated>2015-12-23T13:47:18Z</updated>

		<summary type="html">&lt;p&gt;创建页面，内容为“The K-z relation for radio galaxies *a tight relationship between their near-infrared K-band magnitudes and their radio luminosities *host galaxies of powerful radio...”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The K-z relation for radio galaxies&lt;br /&gt;
*a tight relationship between their near-infrared K-band magnitudes and their radio luminosities&lt;br /&gt;
*host galaxies of powerful radio sources have a fairly small scatter in luminosity&lt;br /&gt;
*leading to the `K-z relation’ or `near-infrared Hubble diagram’&lt;br /&gt;
*http://astroherzberg.org/people/chris-willott/research/k-z-relation/&lt;/div&gt;</summary>
		<author><name>Shen</name></author>
	</entry>
</feed>