Argon X-ray absorption in the local ISM

We present the first comprehensive analysis of the argon K-edge absorption region (3.1-4.2 \AA) using high-resolution HETGS {\it Chandra} spectra of 33 low-mas X-ray binaries. Utilizing R-matrix theory, we computed new K photoabsorption cross-sections for {\rm Ar}~{\sc i}--{\rm Ar}~{\sc xvi} species...

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Veröffentlicht in:arXiv.org 2024-08
Hauptverfasser: Gatuzz, E, Gorczyca, T W, Hasoglu, M F, García, J A, Kallman, T R
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Gorczyca, T W
Hasoglu, M F
García, J A
Kallman, T R
description We present the first comprehensive analysis of the argon K-edge absorption region (3.1-4.2 \AA) using high-resolution HETGS {\it Chandra} spectra of 33 low-mas X-ray binaries. Utilizing R-matrix theory, we computed new K photoabsorption cross-sections for {\rm Ar}~{\sc i}--{\rm Ar}~{\sc xvi} species. For each X-ray source, we estimated column densities for the {\rm Ar}~{\sc i}, {\rm Ar}~{\sc ii}, {\rm Ar}~{\sc iii}, {\rm Ar}~{\sc xvi}, {\rm Ar}~{\sc xvii} and {\rm Ar}~{\sc xviii} ions, which trace the neutral, warm and hot components of the gaseous Galactic interstellar medium. We examined their distribution as a function of Galactic latitude, longitude, and distances to the sources. However, no significant correlations were discerned among distances, Galactic latitude, or longitude. Future X-ray observatories will allow us to benchmark the atomic data as the main resonance lines will be resolved.
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subjects Argon
Interstellar matter
Longitude
Matrix theory
Observatories
Photoabsorption
Physics - Astrophysics of Galaxies
Physics - High Energy Astrophysical Phenomena
Resonance lines
X ray absorption
X ray binaries
X ray sources
X ray stars
X-ray astronomy
title Argon X-ray absorption in the local ISM
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