AGN luminosity and stellar age -- two missing ingredients for AGN unification as seen with iPTF supernovae
arXiv:1701.08647 · doi:10.3847/1538-4357/aa5d5a
Abstract
Active Galactic Nuclei (AGN) are extremely powerful cosmic objects, driven by accretion of hot gas upon super-massive black holes. The zoo of AGN classes are divided into two major groups, with Type-1 AGN displaying broad Balmer emission lines and Type-2 narrow ones. For a long time it was believed that a Type-2 AGN is a Type-1 AGN viewed through a dusty kiloparsec-size torus, but an emerging body of observations suggests more than just the viewing angle matters. Here we report significant differences in supernova counts and classes in the first study to date of supernovae near Type-1 and Type-2 AGN host galaxies, using data from the intermediate Palomar Transient Factory, the Sloan Digital Sky Survey Data Release 7 and Galaxy Zoo. We detect many more supernovae in Type-2 AGN hosts (size of effect 5.1) compared to Type-1 hosts, which shows that the two classes of AGN are located inside host galaxies with different properties. In addition, Type-1 and Type-2 AGN that are dominated by star formation according to WISE colours and are matched in 22 m absolute magnitude differ by a factor of ten in [OIII]5007 luminosity, suggesting that when residing in similar type of host galaxies Type-1 AGN are much more luminous. Our results demonstrate two more factors that play an important role in completing the current picture: the age of stellar populations and the AGN luminosity. This has immediate consequences for understanding the many AGN classes and galaxy evolution.
Accepted to the Astrophysical Journal (ApJ)
References in corpus (16)
- The Host Galaxies and Classification of Active Galactic Nuclei
- Galaxy Zoo 1 : Data Release of Morphological Classifications for nearly 900,000 galaxies
- Determining the Type, Redshift, and Age of a Supernova Spectrum
- The Star-Forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC3227
- Fueling AGN II: Spatially Resolved Molecular Inflows and Outflows
- Multi-phase Nature of a Radiation-Driven Fountain with Nuclear Starburst in a Low-mass Active Galactic Nucleus
- The MIXR sample: AGN activity versus star formation across the cross-correlation of WISE, 3XMM, and FIRST/NVSS
- Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
- The Core Collapse Supernova Rate from the SDSS-II Supernova Survey
- The different neighbours around Type-1 and Type-2 active galactic nuclei
- Supernovae and their host galaxies - II. The relative frequencies of supernovae types in spirals
- On the dichotomy of Seyfert 2 galaxies: intrinsic differences and evolution
- Studying the evolution of galaxies in compact groups over the past 3 Gyr. I. The nuclear activity
- A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
- Comparing narrow and broad-line AGNs, in a new diagnostic diagram for emission-line galaxies based on WISE data
- Does the Jet Production Efficiency of Radio Galaxies Control Their Optical AGN Types?
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- The radio detection and accretion properties of the peculiar nuclear transient AT 2019avd
- The XXL Survey XIX. A realistic population of simulated X-ray AGN: Comparison of models with observations
- Morphology of Seyfert Galaxies
- Examining supernova events in Type 1 active galactic nuclei