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SUMMARY:Chemo-dynamical modelling of galaxies with DYNAMITE
DTSTART;VALUE=DATE-TIME:20230320T133000Z
DTEND;VALUE=DATE-TIME:20230320T134500Z
DTSTAMP;VALUE=DATE-TIME:20240704T115716Z
UID:indico-contribution-186@meetings.aip.de
DESCRIPTION:Speakers: Alice Zocchi (University of Vienna)\nThe combination
  of astrometric and chemical information from Galactic stars has revealed 
 great detail about the structure\, dynamics and history of our own Galaxy.
  In external galaxies\, it is impossible to map the distribution of indivi
 dual stars\, but high signal-to-noise integral field spectroscopy data at 
 various wavelengths\, together with sophisticated dynamical models\, give 
 us the opportunity to gather information on the structure\, dynamics and h
 istory of these systems.\nI will present the Schwarzschild code DYNAMITE (
 https://dynamics.univie.ac.at/dynamite_docs/index.html)\, which models gal
 actic dynamics by means of a superposition of stellar orbits. DYNAMITE is 
 equipped to deal with very detailed kinematic measurements\, allowing us t
 o better exploit high-quality IFU datasets of nearby galaxies. I will prov
 ide a detailed overview of the challenges of such a modelling technique an
 d introduce first applications on observations and simulations. I will als
 o show how DYNAMITE makes it possible to identify families of orbits origi
 nating from different dynamical structures within a galaxy\, which in some
  cases challenge the current picture of galaxies obtained from pure stella
 r light decompositions. Finally\, I will anticipate our future plans for D
 YNAMITE\, adding additional tracers (globular clusters\, extended gas)\, a
 nd dealing with discrete data.\n\nhttps://meetings.aip.de/event/20/contrib
 utions/186/
LOCATION:Haus H\, Telegrafenberg
URL:https://meetings.aip.de/event/20/contributions/186/
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