Conductive Interfaces in Stellar Wind Bubbles

Details Conductive Interfaces in Stellar Wind Bubbles Conductive Interfaces in Stellar Wind Bubbles

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.2492m&link_type=abstract

HST Proposal ID #2492

Physics

Hst Proposal Id #2492

Scientific paper

We propose to observe the conductive interfaces of the stellar wind bubble Sharpless 308 using NV, SiIV and CIV in absorption against the central star HD50896. Our goal is to determine column densities and kinematics in the intermediate temperature gas to help us understand the physics of conductive interfaces. We expect equivalent widths in the range 1-10 mA. We will use the GHRS G160M grating with the A2 mirror to optimize signal and spectral resolution. The data will be modeled with a non-equilibrium ionization code with conductive energy transport.

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