Accretion onto neutron stars can generate photon luminosities well in excess of the Eddington limit. Now it has been shown that it can also produce outflows with similar mechanical power, requiring a rethink of the interaction between accretion flows and neutron star magnetospheres.
References
Belfiore, A. et al. Nat. Astron. https://doi.org/10.1038/s41550-019-0903-z (2019).
Israel, G. L. et al. Science 355, 817–819 (2017).
Fuerst, F. et al. Astrophys. J. 834, 77–84 (2017).
Bachetti, M. et al. Nature 514, 202–204 (2014).
Israel, G. L. et al. Mon. Not. R. Astron. Soc. 466, L48–L52 (2017).
Fuerst, F. et al. Astrophys. J. 831, L14–L19 (2016).
Carpano, S., Haberl, F., Maitra, C. & Vasilopoulos, G. Mon. Not. R. Astron. Soc. 476, L45–L49 (2018).
Weaver, R., McCray, R., Castor, J., Shapiro, P. & Moore, R. Astrophys. J. 218, 377–395 (1977).
Pakull, M. W. & Mirioni, L. Preprint at https://arxiv.org/abs/astro-ph/0202488 (2002).
Pakull, M. W., Soria, R. & Motch, C. Nature 466, 209–212 (2010).
Soria, R., Pakull, M. W., Broderick, J. W., Corbel, S. & Motch, C. Mon. Not. R. Astron. Soc. 409, 541–551 (2010).
Stella, L., White, N. E. & Rosner, R. Astrophys. J. 308, 669–679 (1986).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Soria, R. A pulsar’s shocking power. Nat Astron 4, 119–120 (2020). https://doi.org/10.1038/s41550-019-0934-5
Published:
Issue Date:
DOI: https://doi.org/10.1038/s41550-019-0934-5
- Springer Nature Limited