Cmertin
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I'm trying to understand all the properties of the Jeans instability, the Jeans mass and the Jeans length. I understand the mathematics behind it, though not all the variables. There is a m_{H}[\itex] or I've also seen it as m_{p}[\itex] in the Jeans length and Jeans mass. The formula is as follows:<br />
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M_{J}=(\frac{5×k_{B}×T}{G×μ×m_{H}})^{1.5}×(\frac{3}{4×\Pi×\rho_{0}})^{.5}[\itex], I know that μ is the average molecular mass. &lt;br /&gt;
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Can someone help me understand this please? I&amp;#039;m a bit confused. I tried looking at the units, though couldn&amp;#039;t figure it out.&lt;br /&gt;
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Also, another question about it: Does it work for all masses of ISM? From what I picked up in class, most things don&amp;#039;t work for very large objects in astro, and they need more &amp;quot;fudge factors&amp;quot; to work. Is that the same for the Jeans instabilities?