| Tuesday 13 October
|
| 15.00 - 17.00 |
|
Registration |
| Wednesday 14 October
|
| 08.45 - 09.30 |
Registration |
| 09.30 - 09.45 |
J. Bergeron, J. Mathis |
Introductions |
| 09.45 - 10.25 |
B. Gustafsson |
Chemical abundances of local disk stars |
| 10.30 - 11.00 |
Coffee |
| 11.00 - 11.35 |
D. Lennon |
Massive star abundances |
| 11.35 - 11.50 |
S. Smartt |
New Galactic abundance gradients from early-type stars - the Milky Way and beyond |
| 11.50 - 12.25 |
M. Peimbert |
Galactic HII region abundances |
| 12.25 - 12.40 |
R. Dufour |
C,N,O,Si abundances in the Orion nebula derived from HST FOS UV-optical spectroscopy |
| 12.40 - 14.00 |
Lunch |
| 14.00 - 14.35 |
D. Meyer |
Abundances in interstellar gas |
| 14.35 - 14.50 |
X. Liu |
Abundance determinations of photoionized gaseous nebulae |
| 14.50 - 15.05 |
J. Mathis |
Abundance constraints from interstellar dust |
| 15.05 - 15.55 |
Coffee and Poster Session |
| 15.55 - 16.30 |
A. McWilliam |
Abundances in the Galactic Bulge |
| 16.30 - 17.05 |
F. Matteucci |
Abundance gradients in the Galaxy: a clue to Galaxy formation |
| 17.05 - 17.20 |
A. Ferguson |
Chemical abundances in extreme outer regions of disk galaxies |
| 17.20 - 17.55 |
M. Pettini |
Abundances in damped Lyman-alpha systems |
| 18.00 - 19.30 |
Reception at ESO |
| Thursday 15 October
|
| 09.00 - 09.35 |
B. Pagel |
Chemical evolution of the Magellanic Clouds |
| 09.35 - 10.10 |
E. Skillman |
Backyard cosmology: making abundance observations of nearby galaxies interesting |
| 10.10 - 10.25 |
A. Diaz |
Emipirical calibrations of nebular abundances: The sulphur abundance parameter |
| 10.25 - 10.55 |
Coffee |
| 10.55 - 11.30 |
D. Garnett |
Abundances in spiral and irregular galaxies in the local Universe |
| 11.30 - 11.45 |
C. Henkel |
The detection of extra galactic 15N: Consequences for Nitrogen nucleosynthesis and Chemical Evolution |
| 11.45 - 12.00 |
M. Molla |
Chemical evolution of dwarf galaxies |
| 12.00 - 12.35 |
G. Worthey |
Elliptical galaxy chemical evolution |
| 12.35 - 14.00 |
Lunch |
| 14.00 - 14.30 |
A. Renzini |
Chemical evolution at the galaxy cluster scale |
| 14.30 - 15.05 |
J. Vilchez |
Effects of the environment on star formation and abundances in galaxies |
| 15.05 - 15.45 |
E. Terlevich |
Poster paper review and discussion |
| 15.45 - 16.15 |
Coffee |
| 16.15 - 16.30 |
Y. Izotov |
Heavy element abundances in the most metal deficient blue compact galaxies |
| 16.30 - 16.55 |
C. Leitherer |
Chemical abundances in high-z star-forming galaxies |
| 16.55 - 17.10 |
D. Thomas |
Chemical enrichment of the intracluster medium |
| 17.10 - 17.40 |
F. Combes |
Dust and molecules at high z |
| 17.40 - 17.55 |
V. Dubrovich |
Possible existence of molecules in the shells of quasars 1556+3517 and 0840+3633 |
| Friday 16 October
|
| 09.00 - 09.35 |
A. Songaila
(given by K. Roth) |
Early Metal Formation and the Intergalactic Medium |
| 09.35 - 09.50 |
D. Valls-Gabaud |
Metallicity and massive stars at z~0 and at high redshift: the evolution of the ionising background |
| 09.50 - 10.25 |
F. Thielemann |
Supernova nucleosynthesis: models vs. observations |
| 10.25 - 10.55 |
Coffee |
| 10.55 - 11.10 |
R. Fosbury |
The N/C ratio in high redshift radio galaxies |
| 11.10 - 11.45 |
M. Edmunds
(given by G. Mathlin) |
Dynamical effects on chemical evolution |
| 11.45 - 12.20 |
G. Kauffmann |
The effects of mergers on abundances |
| 12.20 - 12.35 |
V. Kulkarni |
Search for a high-redshift damped Lyman-alpha absorber with NICMOS |
| 12.35 - 14.00 |
Lunch |
| 14.00 - 14.15 |
U. Fritze-
von Alvensleben |
Predicting spectral properties of damped Lyman-alpha galaxies |
| 14.15 - 14.50 |
M. Haehnelt |
Chemical evolution of the intergalactic gas |
| 14.50 - 15.30 |
Discussion - |
Can we trust chemical abundances at z>5? |
| 15.30 - 16.00 |
Coffee |
| 16.00 - 16.20 |
E. Jenkins |
Present and forthcoming UV missions |
| 16.20 - 16.40 |
S. D'Odorico |
Measuring chemical abundances with the VLT instruments |
| 16.40 - 17.00 |
S. Kahn |
Abundance determinations through astrophysical X-ray spectroscopy |
| 17.00 - 17.20 |
N. Thatte |
Increasing abundance of infrared observing facilities |
| 17.20 - 17.40 |
K. Menten |
Abundance measurements with the next generation of radio and (sub)mm instruments |
| 17.40 - 18.10 |
S. White |
Conference summary |
