| Issue |
A&A
Volume 688, August 2024
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Astrophysical processes | |
| DOI | https://doi.org/10.1051/0004-6361/202450732e | |
| Published online | 30 July 2024 | |
Congruity of the Crab Pulsar’s γ-ray spectrum with the spectral distribution of tightly focused caustics (Corrigendum)
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
e-mail: ardavan@ast.cam.ac.uk
Key words: pulsars: individual: J0534+2200 / gamma rays: stars / stars: neutron / methods: data analysis / radiation mechanisms: non-thermal / errata / addenda
The labels on the vertical axes of Figs. 8 and 9 should read “log [Frequency × Flux (erg cm−2 s−1)]”. See the sequels to this paper (Ardavan 2024a,b) for updated accounts of the congruity of pulsars’ spectra with the spectral distribution of the caustics generated by the current sheet in their magnetosphere.
References
- Ardavan, H. 2024a, JCAP, 05, 067 [CrossRef] [Google Scholar]
- Ardavan, H. 2024b, MNRAS, 529, 3744 [NASA ADS] [CrossRef] [Google Scholar]
© The Authors 2024
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