Disentangling the physical parameters of gaseous nebulae and galaxies

Daichi Kashino, Akio K. Inoue

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

We present an analysis to disentangle the connection between physical quantities that characterize the conditions of ionized H ii regions-metallicity (Z), ionization parameter (U), and electron density (ne)-and the global stellar mass (M) and specific star formation rate (sSFR = SFR/M) of the host galaxies. We construct composite spectra of galaxies at 0.027 ≤ z ≤ 0.25 from Sloan Digital Sky Survey, separating the sample into bins of M and sSFR, and estimate the nebular conditions from the emission-line flux ratios. Specially, metallicity is estimated from the direct method based on the faint auroral lines [O iii]λ4363 and [O ii]λλ7320,7330. The derived metallicities cover a range of 12 + log O/H ∼7.6-8.9. It is found that the three nebular parameters, Z, U, and ne, are tightly correlated with the location in the M-sSFR plane. With simple physically motivated ansätze, we derive scaling relations between these physical quantities by performing multiregression analysis. In particular, we find that U is primarily controlled by sSFR, as U∝sSFR0.43, but also depends significantly on both Z and ne. The derived partial dependence of U∝Z-0.36 is weaker than the apparent correlation (U∝Z-1.52). The partial dependence of U on ne is found to be U∝ne-0.29. The scaling relations we derived are in agreement with predictions from theoretical models and observations of each aspect of the link between these quantities. Our results provide a useful set of equations to predict the nebular conditions and emission-line fluxes of galaxies in semi-analytic models.

Original languageEnglish
Pages (from-to)1053-1069
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume486
Issue number1
DOIs
Publication statusPublished - 2019
Externally publishedYes

Keywords

  • galaxies: ISM
  • HII regions

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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