Authors:
Feroci M., Casella P., Costa E., Massaro E., Soffitta P., Matt G., Belloni T., Castro-Tirado A.J., Dhawan V., Frontera F., Harmon A., Mirabel F., Pooley G., Tavani M.
Journal:
Astrophysics and Space Science
Abstract:
The galactic superluminal source GRS 1915+105 was observed by BeppoSAX at several occasions from October 1996 to April 2000. In April 1999 the 2-10 keV light curve showed a long series of quasi regular pulses with a recurrence time of about 50 s. Some preliminary results of a spectral analysis are presented.
Keywords:
Accretion disk; GRS 1915+105; Microquasar; X-ray sources