An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907.

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Description scientific article published on 20 February 2017
Author/s

author: Andrea De Luca  Daniele D'Agostino  Frank Haberl  Matteo Perri  Andrea Tiengo  Alessandro Papitto  Jörn Wilms  Roberto Turolla  Anna Wolter  David Salvetti  Giovanni Novara  Luca Zampieri  Ruben Salvaterra  Guillermo A Rodríguez Castillo  Gian Luca Israel  Piergiorgio Casella  Luigi Stella  Jochen Greiner  Martino Marelli  Simonetta Puccetti  Andrea Belfiore  Paolo Esposito 

Publication date February 20, 2017
Language English
Country of origin
Wikipedia link
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https://archive.org/details/arxiv-1609.07375

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