<?xml version="1.0" encoding='utf-8'?>
<!DOCTYPE wml PUBLIC "-//WAPFORUM//DTD WML 1.1//EN" "http://www.wapforum.org/DTD/wml_1.1.xml">
<wml>
<card id="card1" title="Ambipolar diffusion - Page 5 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=Ambipolar_diffusion&amp;p=4">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Ambipolar_diffusion&amp;p=6">3.Next</a>
</p>

<p><big> In astrophysics </big></p>
<p>In <a href="page.php?w=astrophysics">astrophysics</a>, "ambipolar diffusion" refers specifically to the <a href="page.php?w=Decoupling_%28cosmology%29">decoupling</a> of neutral particles from plasma, for example in the initial stage of star formation. The neutral particles in this case are mostly <a href="page.php?w=hydrogen">hydrogen</a> molecules in a cloud that would undergo <a href="page.php?w=gravitational_collapse">gravitational collapse</a> if they were not collisionally coupled to the plasma. The plasma is</p><p>
<a accesskey="1" href="page.php?w=Ambipolar_diffusion&amp;p=4">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Ambipolar_diffusion&amp;p=6">3.Next</a>
</p>

<do type="prev" label="Search">
        <go href="search.wml"/>
</do>

</card>
</wml>
