UV view of High Mass X-Ray Binary systems (what we know and perspectives for WSO-UV)
High Mass X-Ray Binary systems (HMXRB) are composed by a compact object orbiting around a OB massive star. The mass transfer which takes place from the massive star onto its compact companion is the responsible of the emission of high energy photons (X-rays) observed in these systems (to which they owe the name of their class). The presence of a
Blay, P.
Fecha de publicación:
9
2011