An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907.
Israel GL, Belfiore A, Stella L, Esposito P, Casella P, De Luca A, Marelli M, Papitto A, Perri M, Puccetti S, Castillo GA, Salvetti D, Tiengo A, Zampieri L, D'Agostino D, Greiner J, Haberl F, Novara G, Salvaterra R, Turolla R, Watson M, Wilms J, Wolter A.
Israel GL, et al. Among authors: marelli m.
Science. 2017 Feb 24;355(6327):817-819. doi: 10.1126/science.aai8635. Epub 2017 Feb 20.
Science. 2017.
PMID: 28219970
Free article.