The nature of LINER galaxies:

Raj Laxmi Singh, Glenn van de Ven, K. Jahnkę, M. Lyubenova, J. Falcón‐Barroso, J. Alves, R. Cid Fernandes, L. Galbany, R. García-Benito, B. Husemann,

Astronomy and Astrophysics · 2013 · 306 citations · 30 references

DOIFull text

Open access

Concepts

Abstract

Context. Galaxies, which often contain ionised gas, sometimes also exhibit a so-called low-ionisation nuclear emission line region (LINER). For 30 years, this was attributed to a central mass-accreting supermassive black hole (more commonly known as active galactic nucleus, AGN) of low luminosity, making LINER galaxies the largest AGN sub-population, which dominate in numbers over higher luminosity Seyfert galaxies and quasars. This, however, poses a serious problem. While the inferred energy balance is plausible, many LINERs clearly do not contain any other independent signatures of an AGN.

References

30