The Mass of the LMXB X-Ray Pulsar X1822-371
The low mass X-ray binary X1822-371 is one of the brightest LMXBs in the optical and it is also the prototypical accretion disc corona source. In spite of it has been widely studied, reliable constraints to the stellar masses have only been set in the last 5 years thanks to the detection of 0.59s X-ray pulses and fluorescent emission lines arising
Muñoz-Darias, Teo et al.
Fecha de publicación:
0
2008