Computer Science – Sound
Scientific paper
Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248...63d&link_type=abstract
X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer
Computer Science
Sound
X-Ray Binary Stars, Spectral Analysis, Interstellar Matter, Doppler Effect, Cosmic Background Radiation, X-Ray Binaries, Analytical Methods Involving Electronic Spectroscopy, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Interaction Of Fluid Motion And Sound, Doppler Effect, And Sound In Flow Ducts, Background Radiations
Scientific paper
High-resolution spectroscopy has recently revealed in many neutron-star Low-Mass X-ray binaries that the shape of the broad iron line observed in the 6.4-6.97 keV range is consistently well fitted by a relativistically smeared line profile. We show here spectral fitting results using a newly developed self-consistent reflection model on XMM-Newton data of the LMXB 4U 1705-44 during a period when the source was in a bright soft state. This reflection model adopts a blackbody prescription for the shape of the impinging radiation field, that we physically associate with the boundary layer emission.
Ballantyne David
D'Aì Antonino
di Salvo Tiziana
Iaria Rosario
Papitto Alessandro
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