To appear in "Chemical Enrichment of the ICM and IGM",
ASP Conference Series, Vol, xxx, 2001, eds. F. Matteucci and
R. Fusco-Femiano.
astro-ph/0107116
Abstract. I provide an observational review of the properties of starburst-driven galactic superwinds, focusing mainly on recent results pertinent to the transport of metals and energy into the IGM. Absorption-line studies are providing rich kinematic information on both neutral and ionized gas in superwinds, with observed mass flow rates similar to the star formation rate and outflow velocities comparable to or greater than the escape velocity. FUSE observations of the OVI doublet provide previously unattainable information regarding outflow velocities and radiative cooling rates in hot gas at T ~ 3 × 105 K. Emission from gas at temperatures of 104 K and ~ 5 × 106 K is now being studied with unprecedented spatial resolution using HST and Chandra, tracing the complex interaction of the still-invisible wind of SN-ejecta with the ambient ISM entrained into these outflows. I discuss the implications of these observations for our understanding of starburst-driven outflows.
INTRODUCTION
STARBURST GALAXIES IN THE LOCAL UNIVERSE
THE EFFICIENCY OF SUPERNOVA HEATING
WARM NEUTRAL GAS IN SUPERWINDS
WARM IONIZED GAS
UV ABSORPTION PROBES OF CORONAL GAS
THERMAL X-RAY EMISSION FROM SUPERWINDS
SUMMARY AND CONCLUSIONS
REFERENCES
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