The optical counterparts of Accreting Millisecond X-Ray Pulsars during quiescence
Using data obtained with the ESO-Very Large Telescope, we have performed a deep optical and NIR photometric study of the fields of three Accreting Millisecond X-ray Pulsars (XTE J1814-338, XTE J0929-314 and XTE J1807-294) during quiescence in order to look for the presence of a variable counterpart. If suitable candidates are found, we also carried
D'Avanzo, P. et al.
Fecha de publicación:
10
2008