Discovery of kiloparsec-scale semi-relativistic Fe K$\alpha$ complex emission in NGC 5728

التفاصيل البيبلوغرافية
العنوان: Discovery of kiloparsec-scale semi-relativistic Fe K$\alpha$ complex emission in NGC 5728
المؤلفون: Falcao, Anna Trindade, Fabbiano, G., Elvis, M., Paggi, A., Maksym, W. P., Karovska, M.
سنة النشر: 2023
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
الوصف: We present Chandra ACIS-S imaging spectroscopy results of the extended (1.5''- 8'', 300 pc-1600 pc) hard X-ray emission of NGC 5728, the host galaxy of a Compton thick active galactic nucleus (CT AGN). We find spectrally and spatially-resolved features in the Fe K$\alpha$ complex (5.0-7.5 keV), redward and blueward of the neutral Fe line at 6.4 keV in the extended narrow line region bicone. A simple phenomenological fit of a power law plus Gaussians gives a significance of 5.4$\sigma$ and 3.7$\sigma$ for the red and blue wings, respectively. Fits to a suite of physically consistent models confirm a significance $\geq$3$\sigma$ for the red wing. The significance of the blue wing may be diminished by the presence of rest frame highly ionized Fe XXV and Fe XXVI lines (1.4$\sigma$ - 3.7$\sigma$ range). A detailed investigation of the Chandra ACIS-S point spread function (PSF) and comparison with the observed morphology demonstrates that these red and blue wings are radially extended (~5'', ~1 kpc) along the optical bicone axis. If the wings emission is due solely to redshifted and blueshifted high-velocity neutral Fe K$\alpha$ then the implied line-of-sight velocities are +/- ~0.1c, and their fluxes are consistent with being equal. A symmetric high-velocity outflow is then a viable explanation. This outflow has deprojected velocities ~100 times larger than the outflows detected in optical spectroscopic studies, potentially dominating the kinetic feedback power.
Comment: Accepted for publication on ApJ
نوع الوثيقة: Working Paper
URL الوصول: http://arxiv.org/abs/2303.00782
رقم الأكسشن: edsarx.2303.00782
قاعدة البيانات: arXiv