Comparison of AGN and Nuclear Starburst Activity in Seyfert 1 and 2 Galaxies over a Wide Luminosity Range Based on Near-infrared 2-4 micrometer Spectroscopy
Nagisa Oi (1), Masatoshi Imanishi (2), and Keisuke Imase (1) ((1), GUAS/NAO Japan, (2) NAO Japan)

TL;DR
This study uses near-infrared spectroscopy to compare nuclear starburst activity in Seyfert 1 and 2 galaxies, revealing similar star formation levels relative to AGN power and suggesting star formation influences AGN activity.
Contribution
It introduces a dual-method approach using PAH emission and CO absorption features to assess nuclear starbursts across a wide luminosity range in Seyfert galaxies.
Findings
PAH emission detected in 5 objects
CO absorption detected in 17 objects
Star formation correlates with AGN luminosity
Abstract
We present near-infrared K- (1.9-2.5 micrometer) and L- (2.8-4.2 micrometer) band spectroscopy of 22 Seyfert nuclei. We use two methods to investigate the presence of nuclear starbursts: (1) the Polycyclic Aromatic Hydrocarbon (PAH) emission feature at lambda_rest = 3.3 micrometer in the rest frame of L-band spectrum (a starburst indicator) and (2) the CO absorption feature at lambda_rest = 2.3-2.4 micrometer in the rest frame of the K-band spectrum, originating in the CO molecule. We clearly detected the 3.3 micrometer PAH emission features in five objects and the CO absorption features in 17 objects. Seyfert 2 galaxies tend to show bluer K-L colors compared with Seyfert 1 galaxies. We interpret the discrepancy as resulting from relative strength of stellar emission because AGN emission is affected by dust extinction. The 3.3 micrometer PAH emission luminosity (L_3.3PAH) distributions…
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