A binary pulsar in a 53-minute orbit

Spider pulsars are neutron stars that have a companion star in a close orbit. The companion star sheds material to the neutron star, spinning it up to millisecond rotation periods, while the orbit shortens to hours. The companion is eventually ablated and destroyed by the pulsar wind and radiation(1...

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Detalles Bibliográficos
Autores principales: Pan, Z., Lu, J. G., Jiang, P., Han, J. L., Chen, H.-L., Han, Z. W., Liu, K., Qian, L., Xu, R. X., Zhang, B., Luo, J. T., Yan, Z., Yang, Z. L., Zhou, D. J., Wang, P. F., Wang, C., Li, M. H., Zhu, M.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10468392/
https://www.ncbi.nlm.nih.gov/pubmed/37339734
http://dx.doi.org/10.1038/s41586-023-06308-w

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10468392/
https://www.ncbi.nlm.nih.gov/pubmed/37339734
http://dx.doi.org/10.1038/s41586-023-06308-w

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