NGC 7314: X-ray Study of the Evolving Accretion Properties

TL;DR

This study analyzes X-ray observations of NGC 7314, revealing variable accretion properties, distinct emission regions, and evidence of a changing-state active galactic nucleus through spectral and timing analysis.

Contribution

It provides a comprehensive multi-instrument X-ray analysis showing evolving accretion features and emission components in NGC 7314, highlighting its potential as a changing-state AGN.

Findings

Variable soft and hard X-ray emission origins identified.

Detection of broad and narrow Fe Kα emission lines.

Evidence of evolving spectral properties over time.

Abstract

We present a comprehensive analysis of the timing and spectral properties of NGC 7314, a Seyfert 1.9 galaxy, using X-ray observations from {\it XMM-Newton}, {\it NuSTAR}, and {\it RXTE}/PCA. The timing analysis reveals significant variability across different energy bands, with fractional variability (F$_{\rm var}$) values consistent with previous studies. The highly variable soft photons and comparatively less variable high energy photons imply different origins of these two types. The soft energy photons come from a hot corona near the center, while the high-energy photons are produced by inverse Compton scattering of these primary X-ray photons in a hot plasma away from the central region. The spectral analysis employs various models to characterize the emission components. The results indicate the presence of a soft energy bump, Fe K$\alpha$ line emission, and a prominent reflection component. The long-term {\it RXTE}/PCA data analysis reveals temporal variations in the photon index ($\Gamma$) and power-law flux, suggesting evolving emission properties over time. The signature of both broad and narrow Fe~K$\alpha$ emission line features suggested the broad, variable one coming from the accretion disk ($\sim10^{-5}$~pc), while the non-evolving narrow line can not be well constrained. The absorption feature could originate in a highly ionized region, possibly closer to the broad-line region (BLR). The evolution of the inner accretion properties indicates that NGC 7314 could be a potential changing-state active galactic nuclei.