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Deep Chandra Observations of ESO 428-G014: IV. The Morphology of the Nuclear Region in the Hard Continuum and Fe Kα Line
G. Fabbiano, A. Siemiginowska, A. Paggi +7
We report the results of high-resolution subpixel imaging of the hard continuum and Fe Kα line of the Compton Thick (CT) Active Galactic Nucleus (AGN) ESO 428-G014, observed with C…
CHEERS Results from NGC 3393, III: Chandra X-ray Spectroscopy of the Narrow Line Region
W. Peter Maksym, Giuseppina Fabbiano, Martin Elvis +6
We present spatially resolved Chandra narrow-band imaging and imaging spectroscopy of NGC 3393. This galaxy hosts a Compton-thick Seyfert 2 AGN with sub-kpc bipolar outflows that a…
Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. II. Spatially Resolved Mass Outflow Rates for the QSO2 Markarian 34
Mitchell Revalski, D. Dashtamirova, D. M. Crenshaw +10
We present spatially resolved mass outflow rate measurements () for the narrow line region of Markarian 34, the nearest Compton-thick type 2 quasar (QSO2). Spectra ob…
Deep Chandra Observations of ESO 428-G014: III. High Resolution Spectral Imaging of the Ionization Cone and Radio Jet Region
G. Fabbiano, A. Paggi, M. Karovska +3
We have analyzed the deep Chandra observation (~155 ks) of the Compton Thick Active Galactic Nucleus (CT AGN) ESO 428-G014, to study in detail the morphology of the diffuse X-ray e…
Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array
Kristina Nyland, Jeremy J. Harwood, Dipanjan Mukherjee +19
Energetic feedback by Active Galactic Nuclei (AGNs) plays an important evolutionary role in the regulation of star formation (SF) on galactic scales. However, the effects of this f…
Deep Chandra Observations of ESO 428-G014: II. Spectral Properties and Morphology of the Large-Scale Extended X-ray Emission
G. Fabbiano, A. Paggi, M. Karovska +4
We present a deep Chandra spectral and spatial study of the kpc-scale diffuse X-ray emission of the Compton thick (CT) AGN ESO428-G014. The entire spectrum is best fit with composi…