A Method for Measuring Variations in the Stellar Initial Mass Function
Calzetti, D.; Kennicutt, R. C.; Lee, J. C.; Chandar, R.; Elmegreen, B. G.; Whitmore, B.
United States, United Kingdom
Abstract
We present a method for investigating variations in the upper end of the stellar initial mass function (IMF) by probing the production rate of ionizing photons in unresolved, compact star clusters with ages <=107 yr and with different masses. We test this method by performing a pilot study on the young cluster population in the nearby galaxy NGC5194 (M51a), for which multi-wavelength observations from the Hubble Space Telescope are available. Our results indicate that the proposed method can probe the upper end of the IMF in galaxies located out to at least ~10 Mpc, i.e., a factor ≈200 further away than what is possible by counting individual stars in young compact clusters. Our results for NGC5194 show no obvious dependence of the upper mass end of the IMF on the mass of the star cluster down to ≈103 M sun, although more extensive analyses involving lower mass clusters and other galaxies are needed to confirm this conclusion.
Based on archival data (GO-10452 and GO-10501) of observations obtained with the Hubble Space Telescope, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.