Computer Science
Scientific paper
Sep 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459..437r&link_type=abstract
In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:
Computer Science
Accretion, Accretion Disks, X-Rays: Stars
Scientific paper
We have established the hard X-ray spectral characteristics of the Galactic micro-quasar GRS 1915+105 using the RXTE archives. We make a combined fit to the PCA and HEXTE data and derive the spectral parameters in the low-hard and high-soft states of the source. We resolve the X-ray spectra into three components namely: a multi-color disk component, a Comptonized component and a power-law at higher energies. We find that the spectral states are defined by the relative importance of each of these components. We find a distinct X-ray spectral difference between the radio-loud and radio-quiet low-hard states of the source.
Rao Ravi A.
Vadawale Santosh V.
No associations
LandOfFree
Hard X-ray spectrum of GRS 1915+105: the disk-jet connection does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Hard X-ray spectrum of GRS 1915+105: the disk-jet connection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hard X-ray spectrum of GRS 1915+105: the disk-jet connection will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1489179