Abstract
We report the discovery of a rare compact early-type galaxy, SDSS J085431.18+173730.5 (hereafter cE-AGN). It has a half-light radius of Re =490 pc and a brightness of Mr =-18.08 mag. Optical spectroscopy available from the Sloan Digital Sky Survey (SDSS) reveals the presence of prominent broad-line emissions with the Hα broad component width of FWHM =2400 km s-1. The black hole (BH) mass, as estimated from the luminosity and width of the broad Hα emission, is 2.1x106. With the help of surface photometry, we perform a detailed analysis of the structural properties. The observed light distribution is best modeled with a double Sérsic function. Fixing the outer component as an exponential disk, we find that the inner component has a Sérsic index of n =1.4. Considering the inner component as bulge/spheroidal we find that cE-AGN remains consistent in both the BH mass-bulge mass relation and the BH mass-bulge Sérsic index relation. Given these observational properties, we discuss its possible origin investigating the surrounding environment where it is located.
| Original language | English |
|---|---|
| Article number | L19 |
| Journal | Astrophysical Journal Letters |
| Volume | 820 |
| Issue number | 1 |
| DOIs | |
| State | Published - 20 Mar 2016 |
Keywords
- galaxies: active
- galaxies: bulges
- galaxies: dwarf
- galaxies: elliptical and lenticular, cD
- galaxies: individual (SDSS J085431.18+173730.5)
- galaxies: stellar content
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