ASTRO 358 (UNIQUE 49520)/SPRING 2008 GALAXIES AND THE UNIVERSE COURSE OUTLINE I will try to adhere to the course calendar below as closely as possible, but there may be small changes, based on the course feedback. A reading list is given at the end. The most current version of the calendar can be found at http://www.as.utexas.edu/~sj/a358-sp08/a358-sp08-calendar.txt === Tu Jan 15 + Th Jan 17 Read pre-requisite material emailed to class Review session on background pre-requisite material. === Tu Jan 22 + Th Jan 24: Introduction Types of Galaxies Classification schemes: Hubble-Sandage, RC3, etc === Tu Jan 29 + Th Jan 31 Galaxy Distributions: Field, Groups, Clusters Galaxy Luminosity functions === Tu Feb 05 Stellar Populations and Star Formation History of Galaxies === Th Feb 07 IN-CLASS QUIZ ON MATERIAL COVERED TO DATE === Tu Feb 12 Stellar Populations and Star Formation History of Galaxies === Th Feb 14 Tracing Dark Matter in Galaxies === Tu Feb 19 + Th Feb 21 Tracing Dark Matter in Groups and Clusters Candidates for Dark Matter Modes of structure formation in CDM vs HDM models Dark Matter vs Dark Energy === Tu Feb 26 + Th Feb 28 LCDM models: a first introduction SB profile and kinematics of E, Sp === Th Feb 28 Galaxy Interactions/Mergers: Impact on SF, AGN activity, structure === Tu Mar 04 Galaxy Interactions/Mergers: Major and Minor mergers Review session === Th Mar 06 FIRST EXAM === Tu Mar 11 + Th Mar 13 Spring Break === Tu Mar 18 Hierarchical formation of Spirals and Ellipticals in LCDM models Successes of LCDM-based models of galaxy evolution Challenges/Failures of LCDM-based models of galaxy evolution === Th Mar 20 Star formation tracers - Lyman Continuum Photons (L<912 A; far UV) - Hydrogen Recombination Lines (Ly-alpha, Halpha, Pa-alpha, Br-gamma) - Thermal Radio continuum - Non Thermal Radio Continuum - Far-IR continuum - Mid-IR emission === Tu Mar 25 Star formation tracers (contd) === Th Mar 27 Criteria for onset of star formation - Toomre Criterion for gravitional instability. - Application in outer disks - Application in central region of galaxies ===Tu Apr 01 Star formation law: Schmidt Law. Feedback from star formation and black holes Cosmic SF history and Madau plot === Th Apr 03 IN-CLASS QUIZ Cosmology basics: Redshift, Lookback time and Angular Diameter Distance == Tu Apr 08 + Th Apr 10 Galaxy surveys through cosmic time: the empirical approach to galaxy evolution -- Important criteria for a powerful galaxy survey -- Latest Galaxy Surveys: GEMS, HUDF -- What have we learnt from galaxy surveys at different z? == Tu Apr 15 + Th Apr 17 Galaxy surveys through cosmic time: the empirical approach to galaxy evolution -- Important criteria for a powerful galaxy survey -- Latest Galaxy Surveys: GEMS, HUDF -- What have we learnt from galaxy surveys at different z? == Tu Apr 15 + Th Apr 17 Black Holes and Galaxy Evolution - Rs and Rgrav - Angular momentum problem in fueling BHs - Energy generated by mass accretion onto a BH - Eddington Luminosity - BH Mass vs Bulge vel dispersion relation - Possible reasons for BH Mass vs Bulge vel dispersion relation - Role of AGN feedback on galaxy evolution === Tu Apr 22 Scaling Relations in Galaxies -Tully Fisher relation in spirals -Baryonic Tully Fisher relation in spirals -Faber Jackson in Es -Fundamental plane of Es === Th Apr 24 Epilogue === Tu Apr 29 Student talks Future facilities and challenges === Th May 01 SECOND EXAM READING - GU = "Galaxies in the Universe: An Introduction", by Sparke & Gallagher (Publisher: Cambridge University Press, copyright 2000) - EAC = "Extragalactic Astronomy and Cosmology" by Peter Schneider (Publisher: Spinger, copyright 2006) - GA = "Galactic Astronomy, by Binney and Merrifield (Publisher: Princeton University Press, copyright 1998)