TY - JOUR
T1 - Erratum
T2 - A burst in a wind bubble and the impact on baryonic ejecta: High-energy gamma-ray flashes and afterglows from fast radio bursts and pulsar-driven supernova remnants (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stw1328)
AU - Murase, Kohta
AU - Kashiyama, Kazumi
AU - Meszaros, Peter
N1 - Publisher Copyright:
© 2017 The Authors.
PY - 2017/6/1
Y1 - 2017/6/1
N2 - The paper 'A burst in a wind bubble and the impact on baryonic ejecta: high-energy gamma-ray flashes and afterglows from fast radio bursts and pulsar-driven supernova remnants' was published in MNRAS, 461, 1498 (2016). We noticed that descriptions on free-free absorption optical depths are not correct. In the text, it was said that the singly ionized state with Text = 105 K is used. But, for the calculation of free-free absorption optical depths in Figs 3 and A1 of the original paper, the fully ionized state with Text = 102.5 K was assumed. The formula used in the numerical code remains valid and the conclusions of Murase, Kashiyama &Meszáros (2016) do not change even with more realistic values. However, we here present additional plots, in which free-free optical depths are calculated with more realistic parameters. (Figure Presented).
AB - The paper 'A burst in a wind bubble and the impact on baryonic ejecta: high-energy gamma-ray flashes and afterglows from fast radio bursts and pulsar-driven supernova remnants' was published in MNRAS, 461, 1498 (2016). We noticed that descriptions on free-free absorption optical depths are not correct. In the text, it was said that the singly ionized state with Text = 105 K is used. But, for the calculation of free-free absorption optical depths in Figs 3 and A1 of the original paper, the fully ionized state with Text = 102.5 K was assumed. The formula used in the numerical code remains valid and the conclusions of Murase, Kashiyama &Meszáros (2016) do not change even with more realistic values. However, we here present additional plots, in which free-free optical depths are calculated with more realistic parameters. (Figure Presented).
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U2 - 10.1093/mnras/stx310
DO - 10.1093/mnras/stx310
M3 - Comment/debate
AN - SCOPUS:85090497335
SN - 0035-8711
VL - 467
SP - 3542
EP - 3543
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -