The Mass of the Neutron Star in Cygnus X-2 (V1341 Cygni)
Cygnus X-2 is one of the brightest and longest known X-ray sources. We present high-resolution optical spectroscopy of Cyg X-2 obtained over 4 yr, which gives an improved mass function of 0.69 +/- 0.03 Msolar (1 sigma ). In addition, we resolve the rotationally broadened absorption features of the secondary star for the first time, deriving a
Casares, J. et al.
Fecha de publicación:
1
1998