"Astronomy
with Radioactivities III"
Scientific Program
The Program is being assembled from the contributions offered by participants,
by the organizing team, in early May2001.
Program Components:
-
Stellar Structure in Massive and Giant Stars
-
Core-Collapse SN Models and Nucleosynthesis
-
The s- and r-Process
-
Bolometric Light Curves of Type II Supernovae
-
Novae and 22Na and 26Al
-
Gamma-Ray Lines from 44Ti, 26Al, ...; Positron Annihilation Radiation
-
Chemical Evolution
-
Grains and their Back-Tracing to Novae, r/s-Process etc
-
Dust Formation in Wolf-Rayet Stars, Supernovae
-
Supernova Remnants and their Early Evolution
-
Cosmic Ray Acceleration and Supernova Remnants
-
Instruments for Detection of Cosmic Radioactivities
-
Instruments for Laboratory Analyses of Isotopic Compositions
Program
Details (click here):
For further questions, please contact rod@mpe.mpg.de
History:
- 18 Dec 2000: First version, from responses of first
week