Fall 2000 Galaxy Lunch
 Fridays 12:15 p.m. in 622 Space Sciences 
 Organizers: Martha Haynes, Vassilis Charmandaris 

Note: To join the galaxy lunch mailing list contact Martha Haynes.

Check the lunch talks of Spring 2000 or Fall 1999.

September 1st 

All participants (Cornell University)
Who we are and how we spend our time in the Space Sciences Bldg.
September 8th 
Deparmental Welcome Lunch -- No Galaxy Lunch 
September 15th 
Prof. Martha Haynes (Cornell University) 
``Triggered star formation in the Sco-Cen OB Association'', by Preibisch & Zinnecker Follow this link to see some pictures of the Upper Scorpius OB association. Yes, we consider the Milky Way an interesting galaxy, too!.  
September 22nd 
Renato dall'Acquafredda, Univ. di Buco del Signore  
``The stars near the centre of supergiant shell LMC4: Further constraints on triggering scenarios'', by Braun et al.  
September 29th 
Daniel Devost (Cornell University) 
Overview of the STARBURST 99 code 
October 6th 
John Wilson (Cornell University) 
``Formation of molecular gas in the debris of violent galaxy interactions'', by Braine et al. 
October 13th 
Dr. Thomas Nikola (Cornell University) 
Galaxy collisions and star formation'', by Lamb & Hearn 
October 20th 
Dr. Vassilis Charmandaris (Cornell University) 
``High resolution imaging of molecular gas and dust in the Antennae'', by Wilson et al.  
October 27th 
Barbara Catinella (Cornell University) 
Effects of massive star formation on the ISM of dwarf galaxies'', by Madden  
November 3rd 
JD Smith (Cornell University) 
``Wolf-Rayet stars in starburst galaxies'', by Mas-Hesse et al.  
November 10th 
Chris Springob (Cornell University) 
``Massive star clusters in interacting galaxies'', by Miller  
November 17th 
Laura Hall (Cornell University) 
``A test of arm induced star formation in spiral galaxies from near-IR and Ha imaging'', by Seigar & James  
November 24th 
Thanksgiving Break -- No Galaxy Lunch 
December 1st 
Dr. Bernhard Brandl (Cornell University) 
From NGC3603 to the Antennae: Properties and Evolution of Massive Young Clusters