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X-WR-CALNAME;VALUE=TEXT:ITC Special Seminar - Charles Steinhardt (NBI)
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SUMMARY:ITC Special Seminar - Charles Steinhardt (NBI)
DESCRIPTION:<div>	<span><span><span style="background-color:#ffffff">A Cosmic Ray-Driven Model for Star Formation</span></span></span></div><div>	 </div><div>	<span><span><span style="background-color:#ffffff">Abstract: Observations over the past decade of star-forming galaxies have revealed several surprises, including a similarly in galaxy evolution across a wide variety of conditions and the rapid production of luminous, and presumably massive, galaxies. I will describe these puzzles in more detail, then show a model we have been developing for <span>star formation regulated by a combination of a temperature-dependent initial mass function and heating due to starlight, cosmic rays and, at very high redshift, the cosmic microwave background. This model </span><span>produces an attractor, near-equilibrium solution which is consistent with observations of the star-forming "main sequence" over a broad redshift range. Additional solutions to the same equations may correspond to other observed phases of galaxy evolution including quiescent galaxies. </span></span></span></span></div>
LOCATION:Pratt
STATUS:CONFIRMED
DTSTART:20190117T160000Z
DTEND:20190117T170000Z
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