Effect of dust extinction on estimating the star formation rate of galaxies: Lyman continuum extinction

We reexamine the effect of Lyman continuum (lambda less than or equal to 91 2 Angstrom )extinction (LCE) by dust in H II regions in detail and discuss how it affects the estimation of the global star formation rate (SFR) of ga laxies. To clarify the first issue, we establish two independent methods fo r estimating a parameter of LCE (f), which is defined as the fraction of Ly man continuum photons contributing to hydrogen ionization in an H II region . One of those methods determines f from the set of Lyman continuum flux, e lectron density, and metallicity. In the framework of this method, as the m etallicity and/or the Lyman photon flux increase, f is found to decrease. T he other method determines f from the ratio of infrared flux to Lyman conti nuum flux. Importantly, we show that f less than or similar to 0.5 via both methods in many H II regions of the Galaxy. Thus, it establishes that dust in such H II regions absorbs significant amount of Lyman continuum photons directly. To examine the second issue, we approximate f to a function of o nly the dust-to-gas mass ratio (i.e., metallicity), assuming a parameter fi t for the Galactic H II regions. We find that a characteristic (f) over cap , which is defined as f averaged over a galaxywide scale, is 0.3 for the ne arby spiral galaxies. This relatively small (f) over cap indicates that a t ypical increment factor due to LCE for estimating the global SFR (1/(f) ove r cap) is large (similar to3) for the nearby spiral galaxies. Therefore, we conclude that the effect of LCE is not negligible relative to other uncert ainties of estimating the SFR of galaxies.