1998/09/02 by M. Guainazzi, Guainazzi, M., A. N. Parmar +10
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High-pressure geophysics and materials #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9809014
10 pages, Latex, 9 Postscript figures, accepted for publication in Astronomy & Astrophysics
arxiv created 1998/09/02 · openalex publication_date 1998/09/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We report on the BeppoSAX observation of the X-ray source X1724-308 in the globular cluster Terzan 2. The broadband spectrum can be described as the superposition of a power-law with photon spectral index 1.6-1.9 and a thermal component with typical temperature ~1 keV. X1724-308is detected in the PDS up to 150 keV with a S/N ratio >3, notwithstanding a sharp exponential cutoff at \~90 keV. The broadband spectrum can be best interpreted as due to the Comptonization of a Wien photon distribution with kT ~1 keV by a spherically-symmetric hot plasma with electron temperature ~30 keV and optical depth ~3. A comparison with the fainter and steeper state, which was observed by EXOSAT, suggests a correlation between the temperature of the Comptonizing electron distribution (or the plasma optical depth) and the X-ray intensity. The X-ray thermal component could originate from a boundary layer between the accretion disk and the compact object, or from the accretion disk itself.