Equation (1) in the original paper contained a typographical error and must be replaced by the following (which we slightly reformulated for clarity): (Equation presented). 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.

Salafia, O., Giacomazzo, B. (2022). Corrigendum: Accretion-to-jet energy conversion efficiency in GW170817 (Astronomy and Astrophysics (2021) 645 (A93) DOI: 10.1051/0004-6361/202038590) [Altro] [10.1051/0004-6361/202038590e].

Corrigendum: Accretion-to-jet energy conversion efficiency in GW170817 (Astronomy and Astrophysics (2021) 645 (A93) DOI: 10.1051/0004-6361/202038590)

Salafia O. S.;Giacomazzo B.
2022

Abstract

Equation (1) in the original paper contained a typographical error and must be replaced by the following (which we slightly reformulated for clarity): (Equation presented). 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.
Altro
Erratum
Errata, addenda; Gamma-ray burst: individual: GRB 170817A; Gravitational waves; Relativistic processes; Stars: neutron;
Errata, addenda; Gamma-ray burst: individual: GRB 170817A; Gravitational waves; Relativistic processes; Stars: neutron
English
2022
660
Salafia, O., Giacomazzo, B. (2022). Corrigendum: Accretion-to-jet energy conversion efficiency in GW170817 (Astronomy and Astrophysics (2021) 645 (A93) DOI: 10.1051/0004-6361/202038590) [Altro] [10.1051/0004-6361/202038590e].
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