79
Observational Characteristics
Only one period in power spectra; if this is the orbital period then the secondary has to be degenerate (a white dwarf)
Ramsay et al (2000)
RXJ1914.4+2457
NOT optical data
Cropper et al (1998)
ROSAT HRI data
window
window
window
prewhitened
prewhitened
prewhitened
X-ray
optical