Journal
ASTROPHYSICAL JOURNAL
Volume 654, Issue 1, Pages 494-498Publisher
IOP PUBLISHING LTD
DOI: 10.1086/508744
Keywords
stars : individual (4U 1820-30); stars : neutron; X-rays : binaries; X-rays : stars
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We study the 4-200 keV spectral and temporal behavior of the low-mass X-ray binary 4U 1820 - 30 with INTEGRAL during 2003-2005. This source as been observed in both the soft ( banana) and hard ( island) spectral states. A high-energy tail, above 50 keV, in the hard state has been observed for the first time. This places the source in the category of X-ray bursters showing high-energy emission. The tail can bemodeled as a soft power-law component, with the photon index of similar or equal to 2.4, on top of thermal Comptonization emission from a plasma with electron temperature kT(e) similar or equal to 6 keV and optical depth tau similar or equal to 4. Alternatively, but at a poorer goodness of fit, the hard-state broadband spectrum can be accounted for by emission from a hybrid, thermal-nonthermal, plasma. During this monitoring the source spent most of the time in the soft state, usual for this source, and the greater than or similar to 4 keV spectra are described by thermal Comptonization with kT(e) similar or equal to 3 keV and tau similar or equal to 6-7.
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