Compact elliptical galaxies hosting active galactic nuclei in isolated environment
Soo-Chang Rey, Kyuseok Oh, Suk Kim

TL;DR
This study reports the discovery of active galactic nuclei in nearby isolated compact elliptical galaxies, analyzing their properties and black hole masses to understand their nature and origin.
Contribution
It is the first to identify and characterize AGNs in isolated cEs, estimating black hole masses and confirming their consistency with known scaling relations.
Findings
Four AGNs identified in isolated cEs from SDSS data.
Black hole masses range from 7 x 10^5 to 8 x 10^7 solar masses.
cEs follow established black hole scaling relations.
Abstract
We present the discovery of rare active galactic nuclei (AGNs) in nearby (z < 0.05) compact elliptical galaxies (cEs) located in isolated environments. Using spectroscopic data from the Sloan Digital Sky Survey (SDSS) Data Release 12, four AGNs were identified based on the optical emission-line diagnostic diagram. SDSS optical spectra of AGNs show the presence of distinct narrow-line emissions. Utilizing the black hole (BH) mass-stellar velocity dispersion scaling relation and the correlation between the narrow L([OIII])/L(H\b{eta}) line ratio and the width of the broad H{\alpha} emission line, we estimated the BH masses of the cEs to be in the range of 7 x 10^5 - 8 x 10^7 Msun. The observed surface brightness profiles of the cEs were fitted with a double Sersic function using the Dark Energy Camera Legacy Survey r-band imaging data. Assuming the inner component as the bulge, the K-band…
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