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        <identifier>oai:www.ideals.illinois.edu:2142/18891</identifier>
        <datestamp>2023-07-10</datestamp>
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        <thesis xmlns="http://www.ndltd.org/standards/metadata/etdms/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.ndltd.org/standards/metadata/etdms/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdms11.xsd http://purl.org/dc/elements/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdmsdc.xsd">
          <dc:contributor>Mouschovias, T. Ch.</dc:contributor>
          <dc:creator>Morton, Scott Allyn</dc:creator>
          <dc:date>2011-04-27T15:47:50Z</dc:date>
          <dc:date>2011-04-27T15:47:50Z</dc:date>
          <dc:date>10000-01-01</dc:date>
          <dc:date>1991</dc:date>
          <dc:description>The formation of stars is a fundamental unsolved problem in astrophysics. Interstellar molecular
clouds, observed to be the birth place of stars, have masses much larger than those of typical
stars. Observed densities, temperatures, and strengths of well-ordered magnetic fields imply
that magnetic forces, transmitted to the neutral fluid through collisions with ions, dominate
thermal forces in supporting these objects against self-gravity. The anisotropy of the Lorentz
force, which is always perpendicular to the magnetic field, allows a simplified treatment of the
dynamics involving motion along the magnetic field. We derive a reduced system of non-linear,
non-ideal magnetohydrodynamic equations by assuming a balance of thermal and gravitational
forces along the magnetic field. We then study both the stability of dense clouds as well as
their non-linear evolution/ contraction owing to ambipolar diffusion. An important result is the
selection by ambipolar diffusion of a characteristic mass comparable to a solar mass.</dc:description>
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Original Data
Group with Access UIUC Users [automated]
Release Date: none
Reason: Thesis</dc:description>
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Item is restricted indefinitely.</dc:description>
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          <dc:identifier>3471936</dc:identifier>
          <dc:identifier>http://hdl.handle.net/2142/18891</dc:identifier>
          <dc:language>en</dc:language>
          <dc:rights>1991 Scott Allyn Morton</dc:rights>
          <dc:subject>ambipolar diffusion</dc:subject>
          <dc:subject>interstellar cloud cores</dc:subject>
          <dc:subject>protostars</dc:subject>
          <dc:subject>formation of stars</dc:subject>
          <dc:subject>astrophysics</dc:subject>
          <dc:title>The role of ambipolar diffusion in the formation of interstellar cloud cores and protostars</dc:title>
          <dc:type>Dissertation / Thesis</dc:type>
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            <department>Physics</department>
            <discipline>Physics</discipline>
            <disciplineCode>University of Illinois at Urbana-Champaign</disciplineCode>
            <level>Dissertation</level>
            <name>Ph.D.</name>
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