Physics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1259m&link_type=abstract
HST Proposal ID #1259
Physics
Hst Proposal Id #1259
Scientific paper
We plan to observe supernovae (SNe) brighter than mB ~17m as soon as they are discovered and to follow their evolution in time by means of spectroscopic observations at early epochs and broad band photometry (imaging) at later epochs. Simultaneous IR, optical and radio observations will also be arranged. As interesting side-products, we will be able to study the properties of the intervening gas along the line of sight toward each SN as well as to reveal and study HII regions, bright planetary nebulae and supernova remnants which are expected to be found within the observing slit of the FOC spectrograph. Moreover, we plan to observe some of the brightest SNe which have been discovered recently and whose early phases have been studied by us in great detail.
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