Magellanic Cloud Planetary Nebulae: Cycle 2

Details Magellanic Cloud Planetary Nebulae: Cycle 2 Magellanic Cloud Planetary Nebulae: Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4075b&link_type=abstract

HST Proposal ID #4075

Physics

Hst Proposal Id #4075

Scientific paper

Using the high resolution f/96 mode of the FOC we shall image Magellanic Cloud Planetary Nebulae - objects whose diameters are less than 2 arcsec. Their known distances will allow nebular masses to be derived from their angular diameters, yielding the distribution of PN shell masses for the first time. In combination with their nebular expansion velocities, known from ground-based studies, it will be possible to determine the age of the objects.

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