Graduate Block Lecture Course
Location: ARI Seminarraum
March 27 - April 4, 2008
Lecturers: Eric Bell and Hans-Walter Rix
bell@mpia.de, rix@mpia.de
Scope: This lecture course is the compact equivalent of the semester-long course on galaxies that is established part of the Astronomy/Physics graduate curriculum. The course will convey a broad and up-to date perspective on the current state of knowledge and on the physical principles that shape the properties and evolution of the galaxy population, both at the present epoch and at high redshift. While the cosmological context will be stressed throughout, this class is not a cosmology course, nor has its main focus on modelling galaxy formation. Emphasis will be given to viewing galaxies as 'baryon condensates' in the cosmic dark matter web, to recent quantitative approaches for characterizing the galaxy population properties; there will be focus on the Milky Way and the Local Group - to understand galaxies, when resolved into individual stars; on galaxy dynamics, the role of dark matter in galaxy formation and on black holes at the center; on the various gas phases (and dust) in galaxies. To prepare students for research, the lectures will also discuss the most actively pursued open questions in this field.
Prerequisites: Introduction to Astronomy I and II (or equivalent); basic knowledge of cosmology.
Format:
There will be four lectures each day, 9:00-9:50, 10:00-10:50, 11:00-11:50 amd 13:30-14:20.
One lecture each day (usually 11:00-11:50) will particularly foster active student discussion
and participation, often on the basis of discussion assignments from the previous day.
Lectures
(EFB / HWR)
March 27
Lectures 1+2: Introduction to Galaxies: concepts, history and basic approaches to doing Galaxy Research (pdf)
Lectures 3+4: Brief review of cosmology and the basics of structure formation in cosmology (pdf)
March 28
Lectures 5+6: Research Tools I (pdf)
a) spectral energy distributions
b) interpretation of spectra and colors; masses, SFRs/SFHs, metallicities
Lectures 7+8: Research Tools I (pdf)
c) diagnostics of high z galaxy properties
d) diagnostics of IGM properties (via absorption line spectroscopy)
March 31
Lectures 9+10: Research Tools II (pdf)
e) chemical evolution modeling
f) resolved stellar pops/CMDs
g) diagnostics of ISM and dust
Lectures 11+12: Research Tools II (pdf)
h) dynamics - collisionless/stellar dynamics
i) dynamics - gas
April 1
Lectures 13+14 and 21+22: Cooling, Star Formation and Feedback; Merging and Environment (pdf)
Section on Star Formation (pdf)
April 2
Lectures 15+16: Supermassive black holes, AGN, and AGN feedback (pdf)
Lectures 17+18: Galaxy structures and scaling relations (pdf)
April 3
Lectures 19+20: Galaxy Evolution at z < 1 (pdf)
Lectures 23+24: The Milky Way and the Local Group as a cosmological testbed (pdf)
April 4
Lectures 25+26: High redshift galaxy evolution (pdf)
Final session: discussions, open questions and what new tools will be available soon