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This article is an erratum for:

Volume 649, May 2021
Article Number C4
Number of page(s) 1
Section Astrophysical processes
Published online 07 May 2021

Unfortunately, Eq. (10) in Bosch-Ramon (2021) was incorrectly written. However, the calculations presented in the paper were performed with the correct (approximated) expression for that angle, which is:


where |vw| is the modulus of the stellar wind velocity vector in the orbit-rotating frame, ωorb the pulsar orbital angular velocity, Rorb the orbital separation distance, and η the pulsar-to-star wind momentum rate ratio.


  1. Bosch-Ramon, V. 2021, A&A, 645, A86 [EDP Sciences] [Google Scholar]

© ESO 2021

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