Mj. Coe et al., DISCOVERY OF THE OPTICAL COUNTERPART TO THE CGRO TRANSIENT GRO J1008-57, Monthly Notices of the Royal Astronomical Society, 270(4), 1994, pp. 120000057-120000061
We report observations which identify the optical/LR counterpart to th
e X-ray transient GRO J1008 - 57. The counterpart is shown to be an OB
star with a strong infrared (IR) excess and Balmer emission lines, su
ggesting a Be-type primary. No evidence is found for variability in th
e Ha emission Line over a period of 3 months following the discovery o
f the counterpart in 1993 December.