An assessment of the energy budgets of low-ionization nuclear emission regions

Michael Eracleous, Jason A. Hwang, Hélène M.L.G. Flohic

Research output: Contribution to journalArticle

47 Citations (Scopus)

Abstract

Using the spectral energy distributions (SEDs) of the weak active galactic nuclei (AGNs) in 35 low-ionization nuclear emission regions (LINERs) presented in a companion paper, we assess whether photoionization by the weak AGN can power the emission-line luminosities measured through the large (few-arcsecond) apertures used in ground-based spectroscopic surveys. Spectra taken through such apertures are used to define LINERs as a class and constrain non-stellar photoionization models for LINERs. Therefore, our energy budget test is a self-consistency check of the idea that the observed emission lines are powered by an AGN. We determine the ionizing luminosities and photon rates by integrating the observed SEDs and by scaling a template SED. We find that even if all ionizing photons are absorbed by the line-emitting gas, more than half of the LINERs in this sample suffer from a deficit of ionizing photons. In 1/3 of LINERs the deficit is severe. If only 10% of the ionizing photons are absorbed by the gas, there is an ionizing photon deficit in 85% of LINERs. We disfavor the possibility that additional electromagnetic power, either obscured or emitted in the unobservable far-UV band, is available from the AGN. Therefore, we consider other power sources such as mechanical heating by compact jets from the AGN and photoionization by either young or old stars. Photoionization by young stars may be important in a small fraction of cases. Mechanical heating can provide enough power in most cases but it is not clear how this power would be transferred to the emission-line gas. Photoionization by post asymptotic giant branch stars is an important power source; it provides more ionizing photons than the AGN in more than half of the LINERs and enough ionizing photons to power the emission lines in 1/3 of the LINERs. It appears likely that the emission-line spectra of LINERs obtained from the ground include the sum of emission from different regions where different power sources dominate.

Original languageEnglish (US)
Pages (from-to)796-810
Number of pages15
JournalAstrophysical Journal
Volume711
Issue number2
DOIs
StatePublished - Jan 1 2010

Fingerprint

energy budgets
energy budget
ionization
active galactic nuclei
photoionization
photons
spectral energy distribution
apertures
luminosity
gases
gas
stars
heating
energy
asymptotic giant branch stars
line spectra

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Eracleous, Michael ; Hwang, Jason A. ; Flohic, Hélène M.L.G. / An assessment of the energy budgets of low-ionization nuclear emission regions. In: Astrophysical Journal. 2010 ; Vol. 711, No. 2. pp. 796-810.
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An assessment of the energy budgets of low-ionization nuclear emission regions. / Eracleous, Michael; Hwang, Jason A.; Flohic, Hélène M.L.G.

In: Astrophysical Journal, Vol. 711, No. 2, 01.01.2010, p. 796-810.

Research output: Contribution to journalArticle

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