#  ITC Seminar - Hannah Ubler (MPE) 

 



####  calendar\_today Date and Time 

 **December 10, 2019** 

 12:00PM - 01:00PM EST 

####  pin\_drop Location 

 **Phillips**  



 

 



 

Kinematics of z~1–2 star-forming galaxies with KMOS^3D: intrinsic  
velocity dispersion  
  
Abstract: Kinematics are a powerful tool to study galaxy evolution  
because they are directly affected by transformative processes such as  
accretion, gravitational instabilities, feedback, or outflows. The  
incidence or strength of several of these processes changes with cosmic  
time, allowing us to connect certain kinematic signatures with specific  
physical processes. I will present recent results on the kinematics of  
star-forming galaxies during the peak epoch of cosmic star formation  
from the KMOS^3D survey, with a focus on the redshift evolution of the  
intrinsic velocity dispersion. Combining observational evidence and  
theoretical predictions, I will discuss the origin of the elevated  
velocity dispersions at high redshift.

 

 



 

 See also:- [ 2019 - 20 ](/academic-year/2019-20)
- [ Seminars ](/event-type/seminars)
 
 

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