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PRODID:-//Heidelberg University//HePhySTO//EN
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DTEND:20260821T100000Z
UID:1fe0344add6fcb9afbb40f4aea95e7a2@physik.uni-heidelberg.de
DTSTAMP:20260613T210645Z
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DESCRIPTION:Our unique perspective from within the Milky Way gives us the a
 bility to take images and spectra of individual stars throughout most of th
 e Galaxy. By analyzing this data we have attained a detailed understanding 
 of our Galaxy&apos\;s stellar populations\, gas and dust content\, internal
  dynamics\, and star formation\, chemical enrichment\, and assembly histori
 es. Unfortunately\, this level of detail is somewhat unattainable in extern
 al galaxies due to stellar crowding\, so we must get creative with our anal
 ysis methods to account for this. I will present results from two projects.
  The first involves fitting panchromatic SEDs of resolved stars in two near
 by galaxies that have archival observations from HST and JWST\, which combi
 ne to create the highest resolution broad wavelength coverage possible. Thi
 s provides an incredible opportunity to study dusty star forming galaxies i
 n high resolution\, unveiling why these galaxies are so UV bright for their
  dust content\, and how they form stars despite their low molecular gas mas
 s. The second project involves full-spectrum-fitting of Local Group star cl
 usters from the APOGEE survey. From these high-resolution\, integrated-ligh
 t spectra we can measure the clusters&apos\; kinematics\, metallicities\, a
 nd ? abundances\, which trace the chemical enrichment and assembly history 
 of the galaxy. These two approaches can constrain the assembly and chemical
  enrichment history of nearby galaxies while providing insight into the fun
 damental physics governing galaxy evolution in the nearby universe.\n\nImpo
 rted from https://www.physik.uni-heidelberg.de/hephysto/ (no warranty for a
 ccuracy).
URL;VALUE=URI:https://www.physik.uni-heidelberg.de/hephysto/index.php?s=tal
 k&id=12798
SUMMARY:Königstuhl Colloquium: Ben Gibson - Bridging the Divide: Studying t
 he Resolved and Integrated Light of Nearby Galaxies in High Resolution
DTSTART:20260821T090000Z
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