C. Hellier et al., X-RAY CONFIRMATION OF THE NEW INTERMEDIATE POLAR RX J1238-38, Monthly Notices of the Royal Astronomical Society, 299(3), 1998, pp. 851-854
By finding a 2147-s X-ray pulsation in the recently identified ROSAT s
ource RX 1238-38 we confirm that it is a member of the intermediate po
lar class of cataclysmic variable. We analyse the spectral changes ove
r the white dwarf spin cycle, but are unable to distinguish between co
mpeting mechanisms for the cause of the pulsation. RX 1238-38 has an a
nomalous ratio of spin period to orbital period, similar to that of EX
Hya.