SMC X-2 (SXP2.37) Photometry Revisited

Details SMC X-2 (SXP2.37) Photometry Revisited SMC X-2 (SXP2.37) Photometry Revisited

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1992....1s&link_type=abstract

The Astronomer's Telegram, #1992

Astronomy and Astrophysics

Astronomy

4

Optical, X-Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

SMC X-2 is a transient source, dating back to the earliest X-ray studies
of the Magellanic Clouds (Li et al. 1977, IAU Circ. 3125). During a
bright phase in 2000, Corbet et al. (2001, ApJ 548, L44) discovered
X-ray pulsations with P=2.37 s, but no orbital period has been proposed
using X-ray data (e.g. Galache et al. 2008, ApJS 177, 189).

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