Shaw A.W.; Heinke C.O.; Mukai K.; Tomsick J.A.; Doroshenko V.; Suleimanov V.F.; Buisson D.J.K.; Gandhi P.; Grefenstette B.W.; Hare J.; Jiang J.; Ludlam R.M.; Rana V.; Sivakoff G.R.
(2020)
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. The hard X-ray spectrum of magnetic cataclysmic variables can be modelled to provide a measurement of white dwarf mass. ...