Abstract
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’t Zand 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.
Based on observations collected at the European Southern Observatory, Chile. S.C. thanks Rob Hynes for having alerted him to this new flaring source on September 1999, and Bob Hjellming for the communications he gave on the radio observations. S.C. is very grateful to the ESO/NTT team staff for their availability and skills. S.C. acknowledges support from grant F/00-180/A from the Leverhulme Trust. IFM acknowledges partial support from Conicet/Argentina.
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Chaty, S., Mirabel, I.F., Martí, J., Rodríguez, L.F. (2001). On The Nature of the Microquasar V4641 Sagittarii. In: Castro-Tirado, A.J., Greiner, J., Paredes, J.M. (eds) Microquasars. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0700-9_41
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DOI: https://doi.org/10.1007/978-94-010-0700-9_41
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