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Broad-band X-ray measurements of the black hole candidate XTE J1908+094 | | J.J.M. in ’t Zand
; J.M. Miller
; T. Oosterbroek
; A.N. Parmar
; | | Date: |
30 May 2002 | | Journal: | Astron.Astrophys. 394 (2002) 553-560 | | Subject: | astro-ph | | Affiliation: | Utrecht University and SRON, MIT, ESTEC | | Abstract: | XTE J1908+094 is an X-ray transient that went into outburst in February 2002. After two months it reached a 2-250 keV peak flux of 1 to 2 X 10-8 erg/s/cm2. Circumstantial evidence points to an accreting galactic black hole as the origin of the the X-radiation: pulsations nor thermonuclear flashes were detected that would identify a neutron star and the spectrum was unusually hard for a neutron star at the outburst onset. We report on BeppoSAX and RXTE All Sky Monitor observations of the broad-band spectrum of XTE J1908+094. The spectrum is consistent with a model consisting of a Comptonization component by a ~40 keV plasma (between 2 and 60 keV this component can be approximated by a power law with a photon index of 1.9 to 2.1), a multicolor accretion disk blackbody component with a temperature just below 1 keV and a broad emission line at about 6 keV. The spectrum is heavily absorbed by cold interstellar matter with an equivalent hydrogen column density of 2.5 X 10+22 cm-2, which makes it difficult to study the black body component in detail. The black body component exhibits strong evolution about 6 weeks into the outburst. Two weeks later this is followed by a swift decay of the power law component. The broadness of the 6 keV feature may be due to relativistic broadening or Compton scattering of a narrow Fe-K line. | | Source: | arXiv, astro-ph/0205535 | | Services: | Forum | Review | PDF | Favorites | |
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