X-Ray Absorption Analysis of NGC3516: Appearance of Fast Components with Increased Source Flux
Tomer Holczer, Ehud Behar

TL;DR
This study analyzes Chandra X-ray spectra of NGC 3516 from 2001 and 2006, revealing four distinct outflow components with varying velocities and ionization states, and showing that faster components appear only during higher flux states.
Contribution
The paper identifies four intrinsic outflow components with specific velocities and ionization structures, and demonstrates the appearance of fast components correlating with increased source flux.
Findings
Four outflow components with distinct velocities identified.
Fast components 3 and 4 appear only in high flux state (2006).
Slower components persist across epochs without significant variability.
Abstract
By analyzing the X-ray spectra of NGC 3516 from 2001 and 2006 obtained with the HETGS spectrometer on board the Chandra observatory, we find that the kinematic structure of the outflow can be well represented by four outflow components intrinsic to NGC 3516. The outflow velocities of the different components are 350 +-100 km s-1, 1500 +-150 km s-1, 2600 +-200 km s-1 and 4000 +-400 km s-1 for components 1, 2, 3 and 4, respectively. A local component at z = 0 could be confused with intrinsic component 3. Components 1 and 2 have a broad range of ionization manifested by absorption from 23 different charge states of Fe. Component 3 and 4 are more highly ionized and show absorption from only 9 different charge states of Fe, however we were able to reconstruct the absorption measure distribution (AMD) for all four. The total column density of each component is NH = (1.8+- 0.5) X10^22 cm-2, NH…
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