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New Registration & Travel Information Click Here

New (March 7): Full programme Click Here

NEW: Survival Guide; Feb 29, 2008: Click here

New (March 12): All people with a reservation has been assigned a room in our venue Hotel Coral & Marina

New (March 13): If you have a problem, you can reach us at any time to the following cellular phone number +52 1 646 1358052

Important notice. Time zone difference: Be aware that there is a ONE-HOUR difference between California (U.S. side) and Baja California (México side), California being one hour ahead. For those crossing the border, you'll gain an hour.

Galactic Structure and the Structure of Galaxies


March 17-21 2008

Systematic surveys both of the stellar populations of our own Galaxy and of large samples of external galaxies have greatly improved our view of the structure, kinematics, and chemical properties of galaxies. At the same time the establishment of a standard paradigm for the origin and growth of cosmic structure has provided a well-defined framework within which the observed structures are supposed to arise. Despite this, the relative importance and the specific effects of the many physical processes which play a role in shaping galaxies remain controversial.

This conference aims to promote a dialogue between observers studying the structure of our own and other galaxies and theorists trying to understand galaxy formation and evolution in its cosmological context. The focus will primarily be at "low" redshift (z < 1) where the detailed structure of galaxies remains observationally accessible. The conference will last five days (including one half-day) for a total of about 27 hours of talks and it will address the following topics.

High quality JPG image (16" X 24", 6.2 MB) Click Here
PDF file (for normal printing, 328KB) Click Here
 
Topics:

  • Spatial, kinematic and chemical structures in the     Milky Way and other galaxies

  • Fundamental-plane, Tully-Fisher, mass-metallicity-     gas content-SFR, and other scaling relations

  • Relation of galaxy properties to their central     supermassive black holes

  • Relation of galaxy properties to their dark halos and     their larger scale environment

  • Evolution of systematic properties of the galaxy     population to redshift unity

  • Possible links of galaxy structure to assembly and     star formation histories and to the evolution of the DM     distribution

  • Secular evolution versus imprinting at birth; internally     vs externally driven evolution



    Sponsor Institutions:




    Instituto de Astronomía, UNAM




    Max-Planck-Institut fuer Astrophysik
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    Images: Markarian's Chain of galaxies, G. Djorgovski and the Palomar-Quest Survey
    team; Ensenada Bay, L. Aguilar; design, J.C. Yustis
    Desarrollado por NopalWARE © 2007.