Rhd. Corbet et al., The discovery of an outburst and pulsed X-ray flux from SMC X-2 using the Rossi X-ray Timing Explorer, ASTROPHYS J, 548(1), 2001, pp. L41-L44
Rossi X-Ray Timing Explorer (RXTE) All-Sky Monitor observations of SMC X-2
show that the source experienced an outburst in 2000 January-April reaching
a peak luminosity of greater than similar to 10(38) ergs s(-1). RXTE Propo
rtional Counter Array observations during this outburst reveal the presence
of pulsations with a 2.37 s period. However, optical photometry of the opt
ical counterpart shows that the source was still significantly fainter than
it was more than a half a year after the outburst in the 1970s when SMC X-
2 was discovered.