NeV and OIV in Wolf-Rayet Galaxies

Details NeV and OIV in Wolf-Rayet Galaxies NeV and OIV in Wolf-Rayet Galaxies

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30510d&link_type=abstract

Spitzer Proposal ID #30510

Physics

Scientific paper

We propose to investigate the occurrence of the highly excited OIV and NeV lines in a small but well-defined sample of Wolf-Rayet (W-R) galaxies selected from their optical emission lines, starburst size, and abundances. Our observations will help shed more light on the long standing question of the excitation mechanism of OIV in star forming regions. At the same time, we will be able to perform quantitative tests of models predicting the strength of NeV emission in regions solely powered by stars.

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