  We present photometric and spectroscopic optical and near-infrared (NIR)
observations taken during the outburst on September 1999 of the source V4641
Sgr = SAX J1819.3-2525 (in'tzand et al., 2000) = XTE J1819-254 (Markwardt et
al., 1999). We show that our observations suggest a distance between 4 and 8
kpc, the spectral type of the companion star being constrained between B3 and
A2 V, making the system a High Mass X-ray Binary System (HMXB). In view of the
radio and optical/NIR observations, it is possible that the ejecta of the
source interacted with the surrounding medium of the source.
