Physics
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6693n&link_type=abstract
HST Proposal ID #6693
Physics
Hst Proposal Id #6693 Hot Stars
Scientific paper
We propose to exploit the unique spatial resolution of HST to perform a detailed imaging study of three nebulae around Galactic Luminous Blue Variables, selected on the basis of their different morphologies and physical characteristics. The observations will be performed in selected lines and in the continuum, in order to derive a complete picture of the ionized gas and dust distribution within the nebulae, at the same high resolution. Extensive ground based coronographic observations of these nebulae suggest that an interacting wind scenario can explain most of the morphologies observed, both on large and small spatial scales. We want to compare the high resolution HST images with the predictions of multidimensional, hydrodynamical models to quantitatively establish 1} the wind velocity and mass loss properties of the pre outburst phase, and 2} the duration of the pre outburst phase. The large scale nebular structure will provide information on the LBV outburst mechanism and related intervening factors {rotation, binarity}. The small scale features will provide information on the local instabilities, such as anisotropies of the wind. An experiment conducted on recent HST images of the galactic LBV AG Carinae has proven the method is effective and has demonstrated its potential as a diagnostic tool, to empirically investigate the mass loss history and, thereby, the evolutionary history of the central star.
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