Erratum: Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources (Monthly Notices of the Royal Astronomical Society (2021) 503:21 (3540-3551) DOi: 10.1093/mnras/stab670)
Monthly Notices of the Royal Astronomical Society, ISSN: 1365-2966, Vol: 506, Issue: 3, Page: 4446-null
2021
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Correction Description
The paper 'Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources' was originally published in MNRAS, 503, 3540-3551 (2021). The authors regret that fig. 13 as originally published in Chen et al. (2021) did not have a correct chirp mass colour scale. The correct colour scale is shown in Fig. 1 with an updated caption. The sentence in the 10th line of the second paragraph in section 4.7 should accordingly be changed to 'Their pre-UCXB chirp masses are expected to be between 0.36-0.42M⊙'. The quoted values of chirp mass (1.10-1.16M⊙) in conclusion (viii) should also be replaced by 0.36-0.42M⊙. There are no additional effects for the conclusions of the earlier paper.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85119296677&origin=inward; http://dx.doi.org/10.1093/mnras/stab2050; https://academic.oup.com/mnras/article/506/3/4446/6337902; http://academic.oup.com/mnras/article-pdf/506/3/4446/39553287/stab2050.pdf; https://dx.doi.org/10.1093/mnras/stab2050
Oxford University Press (OUP)
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