Emission from dust in galaxies: Metallicity dependence

H. Hirashita, A. K. Inoue, H. Kamaya, H. Shibai

Research output: Contribution to journalArticle

21 Citations (Scopus)

Abstract

Infrared (IR) dust emission from galaxies is frequently used as an indicator of star formation rate (SFR). However, the effect of the dust-to-gas ratio (i.e., amount of the dust) on the conversion law from IR luminosity to SFR has not so far been considered. Then, in this paper, we present a convenient analytical formula including this effect. In order to obtain the dependence on the dust-to-gas ratio, we extend the formula derived in our previous paper, in which a theoretical formula converting IR luminosity to SFR was derived. That formula was expressed as SFR/(M⊙ yr-1) = {3.3 10-10(1 - η)/(0.4 - 0.2f + 0.6ε)}(LIR/L⊙), where f is the fraction of ionizing photons absorbed by hydrogen, ε is the efficiency of dust absorption for nonionizing photons, η is the cirrus fraction of observed dust luminosity, and LIR is the observed luminosity of dust emission in the 8-1000-μm range. Our formula explains the IR excess of the Galaxy and the Large Magellanic Cloud. In the current paper, especially, we present the metallicity dependence of our conversion law between SFR and LIR. This is possible since both f and ε can be estimated via the dust-to-gas ratio, which is related to metallicity. We have confirmed that the relation between the metallicity and the dust-to-gas ratio is applied to both giant and dwarf galaxies. Finally, we apply the result to the cosmic star formation history. We find that the comoving SFR at z ∼ 3 calculated from previous empirical formulae is underestimated by a factor of 4-5.

Original languageEnglish
Pages (from-to)83-90
Number of pages8
JournalAstronomy and Astrophysics
Volume366
Issue number1
DOIs
Publication statusPublished - 2001
Externally publishedYes

Keywords

  • Galaxies: evolution
  • Galaxies: ISM
  • H II regions
  • Infrared: ISM: continuum
  • ISM: dust, extinction
  • Methods: analytical

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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