Expansion and Spectral Softening of the Dust Scattering Rings of GRB 221009A

Abstract

Expanding X-ray halo or rings appear when short pulses of X-ray radiation from a background source are scattered by clouds of dust in the Milky Way. We study the X-ray rings of the brightest gamma-ray burst (GRB) 221009A, detected by the {\it Swift} X-Ray Telescope. The rings center on the GRB position and their angular radii increase with time. We identify five major expanding rings, and our modeling of their expansion history suggests that they are scattered off, respectively, from five dusty clouds at distances of 0.4-13 kpc from the observer. Given an assumed prompt X-ray fluence of this GRB, the fluxes of those rings suggest that these clouds have dust grain column densities of $10^{7\sim 8}\mathrm{c}{\mathrm{m}}^{-2}$. More interestingly, our time-dependent spectral analysis of these rings show that they all experience spectral softening, i.e., getting softer as they expand, with spectral indices ranging from 2.2 to 5, consistent with what the dust scattering model predicts.

9 pages, 6 figures, 2 tables, Accepted for publication in ApJ

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Cited by in corpus (2)

• Probing the interstellar medium toward GRB 221009A through X-ray dust scattering
• The optical constants and grain sizes of interstellar dust measured directly using the dust scattered x-ray halo of GRB 221009A