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DTSTART:20070311T020000
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DTSTART:20071104T020000
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UID:021d835f-2f12-486b-a33a-b0f3e7ba9b47.205613@calendar.missouristate.edu
CREATED:20200131T174323Z
LAST-MODIFIED:20200131T174323Z
LOCATION:Kemper Hall 206
SUMMARY:PAMS Seminar: Dr. Mallory Molina - "Resolving Black Hole and Star-
 Formation Activity in Nearby Galaxies"
DESCRIPTION:Description: Star formation and accreting black holes fundamen
 tally change how a galaxy evolves with time. However\, to fully explain t
 his evolution\, we must understand how small-scale changes affect global 
 properties. \n\n\nThis talk will focus on the spatially resolved sources 
 that power observed emission in other nearby galaxies\, and the dust that
  obscures it. Dr. Mallory Molina will present her work with Hubble Space 
 Telescope data to study the local environment around black holes. She fou
 nd that small-scale shocks significantly contribute to the large-scale em
 ission. She will discuss her work on the obscuration of light from star f
 orming regions. She will compare her results to that from the integrated 
 galaxy light\, and find important differences and relationships between t
 he way dust affects gas and starlight on the two scales.
X-ALT-DESC;FMTTYPE=text/html:&lt;html&gt;&lt;head&gt;&lt;title&gt;&lt;/title&gt;&lt;/head&gt;&lt;body&gt;&lt;p&gt;&lt;e
 m&gt;Description:&lt;/em&gt;&lt;span&gt;&amp;nbsp\;Star formation and accreting black holes 
 fundamentally change how a galaxy evolves with time. However\, to fully e
 xplain this evolution\, we&amp;nbsp\;&lt;/span&gt;must&lt;em&gt;&amp;nbsp\;&lt;/em&gt;&lt;span&gt;underst
 and how small-scale changes affect global properties.&amp;nbsp\;&lt;/span&gt;&lt;/p&gt;\n
 &lt;p&gt;&lt;span&gt;This talk will focus on the spatially resolved sources that powe
 r observed emission in other nearby galaxies\, and the dust that obscures
  it. Dr. Mallory Molina will present&amp;nbsp\;her work with&amp;nbsp\;&lt;/span&gt;&lt;em
 &gt;Hubble Space Telescope&lt;/em&gt;&lt;span&gt;&amp;nbsp\;data to study the local environm
 ent around black holes.&amp;nbsp\;She found that small-scale shocks significa
 ntly contribute to the large-scale emission. She will discuss&amp;nbsp\;her w
 ork on the obscuration of light from star forming regions.&amp;nbsp\;She will
  compare&amp;nbsp\;her results to that from the integrated galaxy light\, and
  find important differences and relationships between the way dust affect
 s gas and starlight on the two scales.&lt;/span&gt;&lt;/p&gt;&lt;/body&gt;&lt;/html&gt;
DTSTART;TZID=America/Chicago:20200206T160000
DTEND;TZID=America/Chicago:20200206T170000
SEQUENCE:3
URL:https://physics.missouristate.edu/seminars.htm
CATEGORIES:Public,Alumni,Current Students,Faculty,Future Students,Staff
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