Conductive Interfaces in Stellar Wind Bubbles Repeat for 2492

Details Conductive Interfaces in Stellar Wind Bubbles Repeat for 2492 Conductive Interfaces in Stellar Wind Bubbles Repeat for 2492

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4782m&link_type=abstract

HST Proposal ID #4782

Physics

Hst Proposal Id #4782

Scientific paper

We propose to observe the conductive interfaces of the stellar wind bubbles in Sharpless 308. This observation will allow us to understand the physics of conductive interfaces. Evaporation in these structures determines both the dynamics of stellar wind bubbles, and the overall mass and energy balance of the interstellar medium. We have chosen nearby bubbles with hot stars within them. We will observe the absorption lines of the ions N V and C IV that occur at the temperatures found in conductive interfaces. We will model the resulting lines with an existing non-equilibrium model of an interface including saturated conduction. This will yield the strength of the evaporation in the interface.

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