BeppoSAX observed GRS1915+105 on October 2000 when the source was mainly in the ρ class characterized by bursts with recurrence time between 40 and 100 s. The X-ray flux showed a general increase during the observation with a complex behavior. We present some results on the time and spectral analysis of MECS and PDS data in time intervals correspondentto a satellite orbit. © 2010 American Institute of Physics.
BeppoSAX observation of the microquasar GRS 1915+105: spectral and timing behavior in the ρ class / MINEO, T; MASSARO, Enrico; CUSUMANO, G.. - 1248:(2010), pp. 183-184. (Intervento presentato al convegno X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES tenutosi a Bologna; Italy nel 7–11 September 2009) [10.1063/1.3475194].
BeppoSAX observation of the microquasar GRS 1915+105: spectral and timing behavior in the ρ class
MASSARO, Enrico;
2010
Abstract
BeppoSAX observed GRS1915+105 on October 2000 when the source was mainly in the ρ class characterized by bursts with recurrence time between 40 and 100 s. The X-ray flux showed a general increase during the observation with a complex behavior. We present some results on the time and spectral analysis of MECS and PDS data in time intervals correspondentto a satellite orbit. © 2010 American Institute of Physics.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
