SECOND ANNOUNCEMENT                      
                                                                   
        ADVANCED LECTURES ON THE STARBURST-AGN CONNECTION         
                                                                      
                    Hosted by the Instituto Nacional de                
                  Astrofísica, Optica y Electrónica (INAOE)                   
                                                                       
               Tonantzintla, Puebla, Mexico June 26-30, 2000          
                                                                       
      
 
 
        Motivation
 
        Over the last two decades our understanding of the physics of active
        galactic nuclei (AGN)  activity  has largely improved. Still the  
        energy source of AGN is a matter of debate. Most models have advanced 
        the idea that the energy source is gravitational and that the ultimate
        evolution of matter into a super-massive black  hole is the cornerstone 
        for further theoretical and observational investigations. On the other 
        hand an alternative scenario has  been put forward to account for the
        activity of radio-quiet AGN. 
 
        Observationally the advent of new space missions has made it possible 
        to gather new information  from wave-bands that are crucial for learning
        about the physical processes originating in or near the nucleus of AGN. 
        For instance, X-rays and masers have revealed large rotational motions  
        around what is apparently a very large  massive object, so centrally
        concentrated that the black hole hypothesis seems to be an unavoidable
        possibility. On the other hand, ground based and HST observations from 
        the UV to the near-IR show that the continuum observed in some Seyfert 2
        galaxies is mainly  generated by a young starburst hence dominated by
        massive stars. Presently it is not only possible to study AGN in many
        different spectral ranges thus providing a very comprehensive picture, 
        but also the gains in spectral and spatial resolution have permitted 
        exploration of the very central regions of AGN in great detail and the 
        links with their host galaxies.
 
        Future progress will come through combining data from innovative 
        instrumentation on large telescopes such as the VLT; and in the future 
        the NGST, the Atacama Large Millimeter Array (ALMA) and the Large 
        Millimeter Telescope (LMT/GTM); together with a theoretical framework 
        which incorporates them into a coherent description. It will be very
        important to see whether the two approaches, the black hole paradigm 
        and the starburst models, can be linked together or excluded in some
        instances. Our recent view  of cosmic evolution over the last 90% of 
        time seems to indicate that AGN may play a role in galaxy formation 
        and evolution, although much  work needs to be done both 
        observationally and theoretically in this domain.
        
  
        Scope
 
        The goal is to gather a team of experts in the field to deliver a 
        thorough review of AGN phenomenology and physics, so as to cover the 
        area and identify the most pertinent outstanding unsolved problems related
        to the starburst-AGN connection. These Lectures are particularly
        dedicated to advanced students, post-docs and researchers. After each
        lecture there will be ample room for discussions. 
 
        The lectures will be held at the Institute campus at Tonantzintla, 
        Puebla.          
 
        Topics to be discussed include:
 
         * Variability
         * Relations between accretion and emission processes in AGN
         * The standard model - Physical Processes
         * Stars in AGN 
         * Fueling the AGN
         * Unified models
         * Cosmic Evolution, Galaxy Formation
 
        Scientific Organizing Committee:
 
           Daniel Kunth (IAP-France)-Chair 
           Itziar Aretxaga (INAOE, Mexico) 
           Horacio Dottori (IFUFRGS, Brazil) 
           Jose Franco (IAUNAM, Mexico) 
           Jorge Melnick (ESO, Chile) 
           Alfonso Serrano (INAOE, Mexico) 
           Guillermo Tenorio-Tagle (INAOE, Mexico) 
           Roberto J. Terlevich (IoA, UK)        

        Invited Lecturers:

           Bradley M. Peterson (Ohio State Univ, USA)
           Suzy Collin (Obs. Meudon, France) 
           Hagai Netzer (Wise Obs., Israel) 
           Roberto J. Terlevich (IoA, UK)
           Francoise Combes (Obs. Meudon, France)
           Robert Goodrich (Keck Obs., USA) 
           Brian J. Boyle (AAO, Australia)


        Local Organizing Committee:

           R. Mújica      (INAOE, chair)
           E. Benítez     (IA-UNAM)
           V. Chavushyan  (INAOE)
           J. Guichard    (INAOE)
           F. Legrand     (INAOE)
           S. Linder      (INAOE)
           D. Mayya       (INAOE)
           S. del Río     (INAOE)
           J.R. Valdés    (INAOE)
           
            
        Lectures Format
   
        Each topic will be covered during about 4 hours in several
        sessions distributed during the week. Participants are encouraged to 
        present their results in poster format. 
        The posters will be displayed permanently during the course in 
        the coffee break area, and there will be ample time for
        discussion of their content.
 
 
        Registration
 
        Registration can be made, either filling in the registration
        form and posting or sending it by Fax to the conference
        center, or by filling in the form on the web-page and sending
        that to us. Registration DEADLINE is April 15th.
 
 
        Abstracts
 
        The abstract for your poster presentation can be sent either by
        e-mail to us or by filling in the appropriate boxes on the
        web-page. 
 

 
   Accommodations 

   We have booked rooms at the housing facilities of the University of Las 
   Americas (UDLA) located in Cholula (10 minutes by car), the closest town to 
   Tonantzintla. We have also made reservations in  two other hotels in Cholula
   (you can have a look to Cholula's map in our web site). Transportation will 
   be available from the Cholula's downtown to Tonantzintla. If you prefer to 
   stay in Puebla, let us know and we will inform you about the options, 
   however, you should take into account that it takes 45 minutes by car to get 
   from Puebla to Tonantzintla. Please fill in the hotel reservation form 
   in the web-page. We will send you confirmation on your hotel reservations. 
 
 
        Meals
        
        Hotel prices include breakfast (except UDLA). Lunch will be served at   
        INAOE, it will cost around 7-8 US$ per meal. For dinner, there are
        several restaurants in Cholula's downtown that are open till late
        at night.
        
        Travelling to Tonantzintla
  
        For instructions on how to get to Tonantzintla, local information
        and pre (post) Conference Travel please check our web page  
 http://www.inaoep.mx/~progharo 
   
 
        Registration Fee
  
        The Advanced Lectures registration fee is 250 US$. You will be required to pay 
        the amount in cash on arrival. We regret that we are NOT able to process 
        credit card payments.
 
 
        The registration fee includes
 
        -  Conference proceedings
        -  Welcoming cocktail
        -  tea/coffee during conference breaks, Monday to Friday
        -  a guided excursion on Wednesday afternoon to historical
           sites around Puebla.
 
 
        
       
         Contact address:
         Secretary of the Guillermo Haro Programme 
         INAOE-Tonantzintla 
         Apdo. Postal 51 y 216 
         Puebla, Pue. C.P. 72000 
         Mexico 
 
         Phone: +52 (2) 2 47 20 11 
         Fax:   +52 (2) 2 47 22 31 
         E-mail: agn00@inaoep.mx 
    http://www.inaoep.mx/~agn00/