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<p>exterior allow the star to contract further. This continues until the gas is hot enough for the internal <a href="page.php?w=pressure">pressure</a> to support the protostar against further gravitational collapse--a state called <a href="page.php?w=hydrostatic_equilibrium">hydrostatic equilibrium</a>. When this accretion phase is nearly complete, the resulting object is known as a <a href="page.php?w=protostar">protostar</a>.<a href="page.php?w=Image%3AN11_%28Hubble%29.jpg">thumb</a>Accretion of material onto the protostar continues partially</p><p>
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