SHINING, A Survey of Far-infrared Lines in Nearby Galaxies. I. Survey Description, Observational Trends, and Line Diagnostics

R. Herrera-Camus, E. Sturm, J. Graciá-Carpio, D. Lutz, A. Contursi, S. Veilleux, J. Fischer, E. González-Alfonso, A. Poglitsch, L. Tacconi, R. Genzel, R. Maiolino, A. Sternberg, R. Davies, A. Verma

Research output: Contribution to journalArticlepeer-review

Abstract

We use the Herschel/PACS spectrometer to study the global and spatially resolved far-infrared (FIR) fine-structure line emission in a sample of 52 galaxies that constitute the SHINING survey. These galaxies include star-forming, active-galactic nuclei (AGNs), and luminous infrared galaxies (LIRGs). We find an increasing number of galaxies (and kiloparsec-size regions within galaxies) with low line-to-FIR continuum ratios as a function of increasing FIR luminosity (L FIR), dust infrared color, L FIR to molecular gas mass ratio (L FIR/M mol), and FIR surface brightness (ΣFIR). The correlations between the [C ii]/FIR or [O i]/FIR ratios with ΣFIR are remarkably tight (∼0.3 dex scatter over almost four orders of magnitude in ΣFIR). We observe that galaxies with and ΣFIR 1011 L o kpc-2 tend to have weak fine-structure line-to-FIR continuum ratios, and that LIRGs with infrared sizes 1 kpc have line-to-FIR ratios comparable to those observed in typical star-forming galaxies. We analyze the physical mechanisms driving these trends in Paper II. The combined analysis of the [C ii], [N ii] 122 μm, and [O iii] 88 μm lines reveals that the fraction of the [C ii] line emission that arises from neutral gas increases from 60% to 90% in the most active star-forming regions and that the emission originating in the ionized gas is associated with low-ionization, diffuse gas rather than with dense gas in H ii regions. Finally, we report the global and spatially resolved line fluxes of the SHINING galaxies to enable the comparison and planning of future local and high-z studies.

Original languageEnglish
Article number94
JournalAstrophysical Journal
Volume861
Issue number2
DOIs
StatePublished - 10 Jul 2018

Keywords

  • galaxies: ISM
  • galaxies: Seyfert
  • galaxies: active
  • galaxies: general
  • galaxies: star formation
  • galaxies: starburst

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