@ARTICLE{2021MNRAS.506.1045M,
       author = {{Middleton}, M.~J. and {Walton}, D.~J. and {Alston}, W. and {Dauser}, T. and {Eikenberry}, S. and {Jiang}, Y. -F. and {Fabian}, A.~C. and {Fuerst}, F. and {Brightman}, M. and {Marshall}, H. and {Parker}, M. and {Pinto}, C. and {Harrison}, F.~A. and {Bachetti}, M. and {Altamirano}, D. and {Bird}, A.~J. and {Perez}, G. and {Miller-Jones}, J. and {Charles}, P. and {Boggs}, S. and {Christensen}, F. and {Craig}, W. and {Forster}, K. and {Grefenstette}, B. and {Hailey}, C. and {Madsen}, K. and {Stern}, D. and {Zhang}, W.},
        title = "{NuSTAR reveals the hidden nature of SS433}",
      journal = {\mnras},
     keywords = {accretion, accretion discs, X-rays: binaries, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2021,
        month = sep,
       volume = {506},
       number = {1},
        pages = {1045-1058},
          doi = {10.1093/mnras/stab1280},
archivePrefix = {arXiv},
       eprint = {1810.10518},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.1045M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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