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==> In this proposal, more time is being requested for MWERNER,WOLFRAYE
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We propose to continue our ISO investigate of Wolf-Rayet (WR) Galaxies
by extending observations to include the OIII 88 micron line. This will
provide an assessment of the ionized gas content in the galaxies,
complementing our other ISO observations which probe the dust and warm
netural gas phase in these objects.  WR galaxies are a subset of emission
line galaxies, harboring bursts of star formation remarkable in both the
degree of formation activity and the short time scales over which the bursts
seem to have occurred.  Our previous ISO observations have detected the CII
158 micron line in two of three galaxies observed, with two galaxies in
the original sample yet to be observed.  In conjunction with ISOPHOT
observations already obtained for these galaxies, which will be used to
determine the luminosity of the starbursts and the dust content of their
parent galaxies, the proposed LWS observations will provide a more
complete understanding of the nature of the interstellar environments
in which these remarkable starbursts occur.