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Eventos Realizados por el Programa Guillermo Haro



2015 Guillermo Haro Wokshop:  "Forming and Fueling Supermassive Black Hole Seeds"


2014 Guillermo Haro School: Advanced School on Integral Field Spectroscopy Techniques and Analysis.


2014 Guillermo Haro Worksop: Observations and Modeling of Circumstellar Disks A Workshop in Memory of Paola D Alessio.


2013: Guillermo Haro Workshop: Galaxy structure and evolution through Integral Field Spectroscopy: the next generation surveys


2013: Guillermo Haro Conference: Massive Young Star Clusters Near and Far: From the Milky Way to Re-ionization


2011: Surveying the gamma-ray sky


2010: Compact superstar clusters, birth, evolution and feedback


2008: Science with SASIR: Sypnoptic All Sky Infrared Survey

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

Última modificación :
09-05-2016 a las 12:11 por LETICIA PORQUILLO RAMOS

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