Programa Internacional de Astrofísica Avanzada
"Guillermo Haro"


Our Forthcoming Event

Guillermo Haro 2011 workshop on High Energy Astrophysic
July 6-15, 2011, Tonantzintla, Puebla, Mexico


The Programme Guillermo Haro
Getting to Puebla Local information
Past events Contact addresses


The Programme


El programa

This Programme is in honor of the remarkable Mexican astronomer Guillermo Haro and will take place at INAOE, an institute founded by Haro, where he carried out most of his astronomical research.

Introduction

Astrophysics is an interdisciplinary science of increasing complexity. Understanding the nature and evolution of astronomical objects and phenomena leads to interrelations between diverse theoretical fields such as high energy physics, nuclear and plasma astrophysics, general relativity, physics of rarefied gases and chaotic dynamic systems, as well as observational techniques spanning the complete electromagnetic spectrum. The study of elementary particles of extremely diverse energies is accomplished by a variety of numerical simulations techniques as a partial substitute to direct experimentation.

Thus, advances in modern astrophysics usually demand interaction amongst researchers of many fields. The collaborations established amongst scientist coming from different fields of astronomy lead to new working procedures enriched by the diversity of ideas from experts with all sorts of astronomical backgrounds. These constitute the basis of any step towards the frontiers of knowledge. Such philosophy can not be alien to the surroundings where it is developed. Experience proves that locations of natural beauty with intense and lively cultural traditions are an incentive towards a wholesome expression in human spirit. The region of Cholula combines its rich cultural tradition with
INAOE's presence, outgrowth of the former Tonantzintla-Tacubaya Astrophysical Observatory which was a cornerstone in the modern history of Mexican Astronomy.

Stimulated by these ideas we propose to create a research programme in advanced astrophysics with the following goals.

Objectives

   1.To create a working atmosphere that favours research in specific topics of Astrophysics,  encouraging collaboration amongst researchers and advanced students.
   2.To promote the development of Astrophysical research at INAOE.

Structure

   1.A Panel will be responsible for the setting of the Programme.
   2.The Panel will carry out the Programme objectives through workshops, conferences and  postdoctoral fellowships oriented towards high standard current astronomical topics.
   3.The Programme will provide the conditions needed for researchers, students and postdoctoral  fellows to meet at INAOE to develop advanced research activities. The Programme will guarantee financial support, computing and library facilities and offices for the efficient work of  simultaneous participation of about 20 scientists.
   4.Participants are expected to stay for a period of not less than 3 weeks.

The Panel

   1.The Panel will consist of internationally renowned scientists.
   2.The Panel functions will be to establish the Programme norms, to choose the topics to be developed within the framework of an annual schedule, to nominate the members to a scientific committee responsible for the annual schedule, to evaluate periodically the Programme results,  to appoint new members to the Programme and to revise and update the Programme objective and policies.
   3.The Panel will appoint one of its members to act as the Executive Secretary who will carry out the Programme policies. His/her functions are detailed below. The Executive Secretary will be in office for 2 years and will be alternated by the Panel members.
   4.The INAOE Director General will be a Panel member.

The Coordinator

The Coordinator's duties are the following:

   1.To represent the Programme.
   2.To solve the logistic and organisative problems related to the workshops and postdoctoral fellowships.
   3.To guarantee that the Panel agreements are meet.
   4.To organise the Panel meetings.
   5.To present an annual report.

Programme Development

   1.The scientific committee appointed by the Panel will design the programme of each event. The scientific committee will be formed by one or more members, and will be responsible for inviting experts in the chosen subject as well as selecting the participants. The Panel will issue partial evaluations about the workshop development suggesting to the Executive Secretary measures neccesary to guarantee the event's success.
   2.The postdoctoral fellowships will span the interval between two consecutive Programme events, never lasting for less than a year. The postdoctoral researchers will participate throughout a complete programme and will be expected to work on the chosen subject.
   3.The programme of each event will include at least one Public Lecture.



 
 
Guillermo Haro


He was a remarkable Mexican intellectual and is best known internationally for his important contributions in the field of Astronomy. In particular, his name is linked to the discoveries of Herbig-Haro objects and blue galaxies, but he also contributed to the growth of other areas of science and technology in Mexico. His professional studies were not in science; rather, he obtained degrees in Law and Philosophy. A lawyer by training, but an astronomer by heart, he devoted great effort to the creation and development of the most important astrophysics research institutes in Mexico today. First, during the fifties and the sixties, he was Director of the Instituto de Astronomía-UNAM, and of the Astrophysical Observatory of Tonantzintla, Puebla. Later, in 1972, he founded and was the first Director of INAOE, located right next to the Observatory in Tonantzintla. With this, he gave a solid push to the fields of Optics and Electronics and, for the first time in the recent history of Mexico, a research and graduate studies center was established outside Mexico City. INAOE has grown steadily, first in Optics and later on in Electronics and Astrophysics, in these 25 years. At present, it is a very active and world renowned center in the three fields.

Professor Haro became member of the prestigious Colegio Nacional in 1953, and was a co-founder of La Academia de la Investigación Científica. These institutions are the most important national academic societies and gather the most important intellectuals of Mexico in all the areas of Science, Technology, Humanities, and Arts. Also, he was one of the main promoters for the transformation of the old Instituto Nacional de la Investigación Científica into the new Consejo Nacional de Ciencia y Tecnología, the organization that distributes federal government grants for basic and technological research, graduate studies programs, and scholarships for Mexican students in foreign countries. Prof. Haro was also a key person in the creation of two important publishing companies originated in Mexico: Fondo de Cultura Económica, and Editores Siglo XXI.


Getting to Puebla

  • Transportation from the Mexico, D.F. airport to Puebla: there is a comfortable bus service by "Estrella Roja" which runs from Mexico City airport to the city of Puebla every 30 minutes. These leave from the airport zone D, next to International Arrivals (zone E). The fare is 198 Pesos (as of June 2010) and is paid in a kiosk located in front the bus departing zone. The ride takes about two hours. Those wanting to see the landscape (once outside Mexico City!) should sit on the right hand side of the bus.
  • Buses departes at several hours arriving at Puebla major bus station (known locally as CAPU) and Terminal 4 Poniente. Please check an update timetable at www.estrellaroja.com.mx. Both Taxis at Terminal 4 Poniente and CAPU have regulated prices, so, after pick up your luggage from the bus, buy the taxi tickets in the designated area (look for the TAXIS sign).
  • From CAPU to INAOE the rides take about 30 minutes and cost about 120 pesos. Tell the taxi driver to drop you at "El Observatorio" in Tonantzintla. If you go to the center ("Puebla centro") just tell the taxi driver the hotel's name.

    Similar prices and times from the "Terminal 4 Poniente". This terminal is better connected with the Airport, nearer to Puebla's downtown, more peaceful and we highly recommend.

  • We strongly advise you against taking taxis from Mexico City airport to Puebla as the fare will be astronomical (at least 1000 pesos).
  • If you are highly adventurous and insist on driving to Tonantzintla, the basic instruction is to go to the city of Puebla (120 kms East), then after entering town head to Cholula (8 kms West) and from there to Tonantzintla (5 kms South). Simple, isn't it? To make life easier, exiting the airport you have to take "boulevard aeropuerto" to the south, after some 3 to 5 kms take "Calzada Ignacio Zaragoza", a wide kind of freeway road, towards the East. After some 15 kms it leads to the beginning of the motorway. Mind: take "Puebla cuota" and NOT" Puebla libre" (a rather bad road).

  • Local information
  • Money:The Mexican currency is the peso ($). The present exchange rate with the U.S. dollar is about $12.0 = 1.0USD, but this changes more rapidly than we would like. Please make sure you have some pesos with you BEFORE leaving the Mexico City airport, where there are plenty of currency exchange offices. Once in Mexico, not all places take US dollars or traveler's checks. Foreign credit cards are accepted in major restaurants, stores, and hotels. Best exchange rates are found in CASAS de CAMBIO (exchange houses) open only on weekdays, usually from 9 am to 5 pm. Most banks open only on weekdays, also from 9 am to 5 pm. The airport has 24 hour money exchange counters. USA cash or travelers checks are easier to change into pesos than other types of currency.
  • Weather: Puebla is located at an altitude of 2200 meters (7100 feet). There is usually no rain during the spring, but it gets rainy during the summer and about the middle of autumn. The temperature varies from some 30 C (85-90 F) in the daytime to about 10 C (50 F) in the night/morning. Note that the air is thin, and it can get cool at night.
  • Language: Spanish is the official language in Mexico. Because Puebla is not overly frequented by tourists, very few people speak English. We advise you to have a good dictionary and a phrasebook when you venture out.


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    Past Events

     

    2010: Compact superstar clusters, birth, evolution and feedback

    2008: Science with SASIR

    2007: The Large Millimeter Telescope: first-light science and future surveys

    2006 International School on Galactic and Cosmological N-Body Simulations

    2006 GH Workshop: Science with the future large Optical/IR facilities in Mexico

    2005 Advanced School: Pan-Chromatic View on Clusters of Galaxies and Large-Scale Structure
    2003 GH  Conference: Multiwavelength AGN Surveys
    2003 GH Workshop: AGN Surveys
    2002 GH Workshop: Millimetre Cosmology: From Primordial Fluctuations to Galaxies
    2001 GH Conference: Disks of Galaxies: Kinematics, Dynamics and Perturbations
    2001 GH Workshop: Disks of Galaxies: Kinematics, Dynamics and Perturbations
    2000 GH Advanced Lectures on the Starburst-AGN Connection
    2000 GH Workshop on the Starburst-AGN Connection
    1999 GH  Conference: Cosmic Evolution and  Galaxy Formation
    1999 GH Workshop:  Large-scale Structure & Clusters of Galaxies
                                              The Energy Input from Stars: Supernovae and
                                               Chemodynamical Evolution
    1998 GH Workshop: The Formation and Evolution of Galaxies
    1998 GH Conference:  Interstellar Turbulence
    1997 GH Workshop: The Physics of Star-Gas Interactions
    1996 GH Conference : Starburst Activity in Galaxies
    1996 GH Workshop: Starburst Galaxies



     

    Contact Addresses

    Guadalupe Rivera Loy


    Last update by danrosa @ inaoep.mx on May 3, 2010