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Continuum Radio Emission from Stars
Up:
SKA Science
Previous:
Magnetic Fields
Formation and Evolution of Stars
Continuum Radio Emission from Stars
Imaging the Surfaces of Stars
Red Giants and Supergiant Stars
Complementarity to Planned Optical-IR Interferometers
Star Formation
Protostellar Cores
Dust around protostars
Dynamics and Chemistry
Protostellar Jets
Uncovering the Evolutionary Sequence
Magnetic Fields in Protostellar Objects
Zeeman Splitting in Molecular Gas
Non-Thermal Emission Processes
Cool Star Astronomy
The Radio Sun
Observing Solar Analogs at Radio Wavelengths
Where are the many other Radio Suns?
Prospects for the SKA
Physics of Solar-Like Stars
Flares and Microflares
Summary of Scientific Objectives
X-ray Binaries
Relativistic Ejections from X-ray Transients
The Faint Persistent Population
The potential of the SKA
Imaging of Circumstellar Phenomena
Stellar Astrometry
Supernovae
Radio Supernovae
New Observations Possible with the SKA
Radio Emission from Type Ia SNe
RSN Distance Determinations
The SN-SNR Connection
Summary and Conclusions
The Radio After-Glows of Gamma-ray Bursts
Pulsars
Pulsar Searches with the SKA
Pulsar Timing with the SKA
Radio Pulsar Timing and General Relativity
Summary
Russ Taylor
1999-06-22
