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Probing The Local Environment of the Supernova Remnant HESS J1731-347 with CO and CS Observations

N. Maxted, M. Burton, C. Braiding, G. Rowell, H. Sano, F. Voisin, M. Capasso, G. Pühlhofer, Y. FukuiMonthly Notices of the Royal Astronomical SocietyPublished Nov 1, 2017doi 10.1093/mnras/stx2727 Original︎ ↗Archived copy

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Assuming standard X-factor values and that most of the HI/CO emission seen towards HESS J1731-347 is on the near-side of the Galaxy, X-ray absorption column densities are consistent with [gas] foreground to, but not beyond, the Scutum-Crux Galactic arm, suggesting a kinematic distance of ~3.2 kpc for HESS J1731-347.

The X-ray absorption column density toward HESS J1731-347 exceeds the total foreground gas column in front of the Scutum-Crux armSupported

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Kind: journal article
Authors: N. Maxted, M. Burton, C. Braiding, G. Rowell, H. Sano, F. Voisin, M. Capasso, G. Pühlhofer, Y. Fukui
Publisher: Monthly Notices of the Royal Astronomical Society
Published: Nov 1, 2017
DOI: 10.1093/mnras/stx2727
Link: https://arxiv.org/abs/1710.06101
Archived copy: https://web.archive.org/web/20251119194636/https://arxiv.org/abs/1710.06101
Stored text: 5,098 characters, retrieved Nov 11, 2026 · 46 sections, 59 passages
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