ITC Pizza Lunches

Spring 2018: Winds and Outflows    Organized by  Antonija Oklopcic and Morgan MacLeod

Spring 2017:  Gravitational Wave Astrophysics  Organized by John Forbes and Dan Milisavljevic 

Spring 2016: Astrostatistics; Organzied by Anna Pancoast and Ilse Cleeves

Spring 2015: Magnetic Fields and Turbulence in Astrophysics

Spring 2014: Time Domain Astronomy; Organized by Sayan Chakraborti and Raffaella Margutti

Spring 2013: Galaxy Clusters; Organized by Cameron McBride

Fall 2012: Dark Matter ; Organized by Matt Walker

Spring 2012: Star Formation and Stellar Dynamics; Organized by Kaitlin Kratter and Smadar Naoz

Fall 2011: Cosmology and Large-Scale Structure; Organized by Charlie Conroy, Debora Sijacki, and Mark Vogelsberge

Spring 2011: Galactic Dynamics; Organized by Hagai Perets, Charlie Conroy, Elena D'Onghia, Mark Vogelsberger, and Mario Juric

Fall 2010: Supernovae; Organized by Alicia Soderberg, Ryan Foley, Hagai Perets

Spring 2010: Formation and Evolution of Planets; Organized by Daniel Fabrycky, Ruth Murray-Clay, and Hagai Perets

Fall 2009: Binaries; Organized by Rosanne Di Stefano and Alicia Soderberg

 

Upcoming ITC Pizza Lunches

2018 Apr 25

ITC Pizza Lunch

11:00am to 12:00pm

Location: 

Phillips
Jeremy Drake (CfA) Stellar Coronal Mass Ejections
Tomek Kaminski (CfA) The role of metal oxides in dust formation around cool evolved stars.
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2018 Apr 11

ITC Pizza Lunch

11:00am to 12:00pm

Location: 

Phillips
Ivan Cabrera (CfA) The gas content of star clusters
Jill Naiman (CfA) Should I Stay or Should I Go: Stellar Wind Retention and Expulsion in Star Clusters
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2018 Mar 28

ITC Pizza Lunch

11:00am to 12:00pm

Location: 

Phillips
Anna Rosen (CfA) The importance of Outflow and Wind Feedback in Massive Star Formation
Atish Kamble (CfA) Radio Supernovae Illuminating the Environments of Massive Stars
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2018 Mar 21

ITC Pizza Lunch

11:00am to 12:00pm

Location: 

Phillips
Sofia Moschou (CfA) Modeling Radio Loud Coronal Mass Ejections
Xiawei Wang (CfA) Non-thermal emission and star formation from AGN outflows
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