The TMR workshop on semi-analytical models of galaxy formation took place on
21/22 March 1997 at the MPA in Munich.

In attendence were:

Kelvin Wu             (IoA, Cambridge)

Carlos Frenk          (University of Durham)
Carlton Baugh
Shaun Cole

Philip Best           (Leiden Observatory)
Huub Rottgering
Amina Helmi

Rosaria Tantalo       (Padova)

Barbara Lanzoni       (IAP, Paris)

Guinevere Kauffmann   (MPA, Munich)
Simon White
Houjun Mo
Shude Mao
Martin Haehnelt
Adi Nusser

Eiichi Egami          (MPE, Munich)

Claudia Maraston      (ESO, Munich)

Bodo Ziegler          (Landessternwarte, Munich)
Paula Belloni



------------------------PROGRAMME----------------------------------------------


FRIDAY, 21 MARCH (MORNING):

 9:30 Guinevere Kauffmann - opening remarks, introduction to the     
			    Munich models

10:00 Houjun Mo  - Analytic methods for estimating correlation funtions  
		   and higher order statistics

10:20 Shude Mao -  Models of disk galaxy formation

10:45-11:15    COFFEE BREAK

11:15 Shaun Cole -  Introduction to the Durham models

11:45 Carlton Baugh - Applications of the Durham models

12:15 Rosaria Tantalo - Chemical evolution and the Padova models 

12:45-2:00     LUNCH

 
FRIDAY, 21 MARCH (AFTERNOON):

The participants divided into two groups. Group 1 consisted of modelling
"experts" (Kauffmann, Cole, Baugh, Mo, Wu). Modelling techniques were
discussed and compared in detail. Kelvin Wu described the new semi-analytic
models being constructed in Cambridge in collaboration with Andy Fabian and
Paul Nulsen.  The Durham modellers described their updated code. It was 
decided that a comparison would be carried out between the Munich, Durham
and Cambridge models. Future projects were outlined.

Group 2 was led by Simon White and Carlos Frenk and was attended mainly by
students and observers wishing to learn more about semi-analytic models
and their capabilities. The format was an informal "question-and-answer" 
session.

FRIDAY NIGHT:
Workshop dinner held at Paulaner an der Au in Munich city centre.


SATURDAY, 22 MARCH :

The whole day was devoted to project discussions. The following topics were
covered.

1) Chemical Evolution: the capabilities of the Padova models, the possibility of
		       introducing the various ingedients of these models into
		       the semi-analytic schemes to study the detailed enrichment
		       history of our own Galaxy and others.

2) The Sizes of Disks: the Munich and Durham groups compared notes on their
		       methods of predicting the evolution of the sizes of galaxies
		       
3) Radio Galaxies: The Munich and Leiden groups discussed plans to model the
		   evolution of the environments of radio galaxies.

4) Comparisons:    A plan for comparing the models of different groups was set up.