Optical excess of ~6 over the
Rayleigh-Jeans tail of the
X-ray best fitting bb (Walter
& Lattimer, 2002)
No X-ray pulsations: upper limit on the pulsed fraction £3% (Ramson
et al, 2002, Drake et al, 2002) Þ
£1% Burwitz
et al., 2002; Trumper , Cospar meeting
d ~120-140 pc (Kaplan et al, 2001; Walter &
Lattimer, 2002) Þ radiation radius of only
5-6 km! (Drake et al, 200