High Resolution Ultraviolet Spectroscopy of Nova Cygni 1992 IN the Nebular Phase

Details High Resolution Ultraviolet Spectroscopy of Nova Cygni 1992 IN the Nebular Phase High Resolution Ultraviolet Spectroscopy of Nova Cygni 1992 IN the Nebular Phase

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.4053s&link_type=abstract

HST Proposal ID #4053

Physics

Hst Proposal Id #4053

Scientific paper

We propose to obtain intermediate dispersion GHRS observations of Nova
Cygni 1992, one of the brightest classical novae of the century. With
this high S/N data, we will study the shell dynamics, shell structure,
and ejecta abundances during the optically thin nebular stages.

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