Key points are not available for this paper at this time.
The clumpy irregular galaxy Mrk 325 contains enormous extranuclear H II- region complexes indicating that Mrk 325 is a starburst galaxy. Scaled- array VLA maps at 1. 49 GHz and 4. 85 GHz show that these H II regions have nonthermal radio spectra, probably because stars more massive than 8 Mₛun_ do not live long enough to escape the H II regions before exploding and creating the supernova remnants responsible for the nonthermal emission. Radio and far-infrared continuum luminosities, hydrogen recombination-line luminosities, and other data were used to constrain the ionization rate NUV_, Type II supernova rate vSN_, and bolometric luminosity Lbol_ of Mrk 325 and of other starburst galaxies. We used a new method to derive much lower values of vSN_ from the nonthermal radio luminosity, thereby avoiding the difficulties or contradictions of earlier models. Most starburst galaxies appear to have similar ratios NUV_/vSN_ and NUV_/Lbol_, suggesting a "universal" initial mass function slope γ ~ 2. 5 for M > 8 Mₛun_ Our starburst model provides a quantitative explanation for the observed correlation between the far-infrared and the (mostly nonthermal) radio continuum flux densities of starburst galaxies.
Condon et al. (1990) studied this question.