Physics
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7837p&link_type=abstract
HST Proposal ID #7837
Physics
Hst Proposal Id #7837 Hot Stars High-Mass Stars
Scientific paper
We image three bright planetary nebulae, which have helium rich stellar atmospheres and helium poor nebulae. However, we think that the inner nebulae must be helium rich on a spatial scale that is very accessible with the NIC1 camera on HST. We would expect the images to show a helium-enriched shell on a scale of app. 1". If observed, this would be the first observation of the changeover from hydrogen rich mass loss to helium rich mass loss in planetary nebulae.
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