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27 April 2024 |
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Hard X-ray emission from Serpens X-1 as observed by INTEGRAL | N. Masetti
; L. Foschini
; E. Palazzi
; L. Amati
; E. Caroli
; G. Di Cocco
; F. Frontera
; M. Orlandini
; | Date: |
21 Mar 2004 | Subject: | astro-ph | Affiliation: | on behalf of a larger collaboration | Abstract: | We here report results of an INTEGRAL observation of the X-ray burst and atoll source Ser X-1 performed on May 2003. The object was observed for a total of 400 ks but nearly 8 degrees off-axis due to the amalgamation with an observation of SS 433, the pointing target source. Ser X-1 was detected up to 30 keV with unprecedented positional accuracy for a high-energy emission; a sharp spectral drop is evident beyond this energy. Significant variability is seen in the 20-30 keV light curve. Comparison with previous observations indicates that the source was in its high (banana) state and displayed a soft spectrum during the INTEGRAL pointing. A (non simultaneous) broadband radio-to-gamma-rays broad-band spectral energy distribution for Ser X-1 is also presented for the first time. | Source: | arXiv, astro-ph/0403505 | Services: | Forum | Review | PDF | Favorites |
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