Understanding the radiative and physical structures of inner region of a few 100 pc of AGNs is important to constrain the causes of their activities. Although the X-ray emission from the Comptonization region/corona and the accretion disc regulates the broad line emission regions and torus structures, the exact mutual dependency is not understood well. We performed correlation studies for X-ray, mid-infrared, and different components of Balmer emission lines for the selected sample of AGNs. Almost 10 different parameters and their inter-dependencies were explored in order to understand the underlying astrophysics. We found that the X-ray luminosity has a linear dependency on the various components of broad Balmer emission lines (e.g. L$_{ \text{ 2-10 keV}}$ $\propto$ L$^{ 0.78}_{ \text{ H}\beta^{ \text{ B}}}$) and found a strong dependency on the optical continuum luminosity (L$_{ \text{ 2-10 keV}}$ $\propto$ L$^{ 0.86}_{ 5100\,\text{ \AA}}$). For a selected sample, we also observed a linear dependency between X-ray and mid-infrared luminosity (L$_{ \text{ 2-10 keV}}$ $\propto$ L$^{ 0.74}_{ 6\,\upmu \text{ m}}$). A break point was observed in our correlation studies for X-ray power-law index, $\Gamma$, and mass of black hole at $\sim$ log (M/M$_{ \odot}$) = 8.95. Similarly the relations between $\Gamma$ and FWHM of H$\alpha$ and H$\beta$ broad components show breaks at FWHM$_{ \text{ H}\alpha}$= 7642$\pm$657 km s$^{ -1}$ and FWHM$_{ \text{ H}\beta}$ = 7336$\pm$650 km s$^{ -1}$. However, more data are required to confine the breaks locations exactly. We noted that $\Gamma$ and Eddington ratios are negatively correlated to Balmer decrements in our selected sample. We analyzed and discussed about the implications of new findings in terms of interaction AGN structures.
Categories: astro-ph.HE astro-ph.GA