Issue |
A&A
Volume 660, April 2022
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/202038590e | |
Published online | 04 April 2022 |
Accretion-to-jet energy conversion efficiency in GW170817 (Corrigendum)
1
INAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy
e-mail: omsharan.salafia@gmail.com
2
INFN – Sezione di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano (MI), Italy
3
Università degli Studi di Milano-Bicocca, Dip. di Fisica “G. Occhialini”, Piazza della Scienza 3, 20126 Milano, Italy
Key words: relativistic processes / gamma-ray burst: individual: GRB 170817A / stars: neutron / gravitational waves / errata, addenda
Equation (1) in the original paper contained a typographical error and must be replaced by the following (which we slightly reformulated for clarity):
The plot in Fig. 4 of the original paper is nevertheless correct: it corresponds to the above formula and not to the one reported in the original paper, which had a wrong coefficient in the first line.
© ESO 2022
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