Search results for "individual : 4U 1705-44"

showing 1 items of 1 documents

BeppoSAX observation of 4U 1705-44: detection of hard X-ray emission in the soft state

2007

4U 1705-44 is one of the best studied type I X-ray burster and atoll sources. Since it covers a wide range in luminosity (from a few to 50 x 10^{36} erg s^{-1}) and shows clear spectral state transitions, it represents a good laboratory to test the accretion models proposed for atoll sources. We analysed the energy spectrum accumulated with BeppoSAX observations (43.5 ksec) in August 2000 when the source was in a soft spectral state. The continuum of the wide band energy spectrum is well described by the sum of a blackbody (kT_{bb}~0.56 keV) and a Comptonized component (seed-photon temperature kT_W~1 keV, electron temperature kT_e~2.7 keV, and optical depth ~11). A hard tail was detected at…

PhysicsPhotonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)stars : individual : 4U 1705-44X-rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsaccretion accretion diskAstrophysicsstars : neutronPower lawK-lineSoft stateSpace and Planetary ScienceX-rays : starElectron temperatureBlack-body radiationEmission spectrumindividual : 4U 1705-44; stars : neutron; X-rays : stars; X-rays : binaries; X-rays : general [accretion accretion disks; stars]X-rays : binarieX-rays : generalAstronomy & Astrophysics
researchProduct