Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...469l..21s&link_type=abstract
Astrophysical Journal Letters v.469, p.L21
Astronomy and Astrophysics
Astronomy
32
Stars: Individual Constellation Name: Circinus X-1, Stars: Neutron, X-Rays: Stars
Scientific paper
We have carried out a study of Cir X-1 through (1) detailed sampling over a single 16.5 day intensity cycle with the Rossi X-Ray Timing Explorer (RXTE) proportional counter array and (2) complementary monitoring over six such cycles with the RXTE all-sky monitor (ASM). We report here the temporal and spectral evolution at nonflaring phases, during which Cir X-1 remained unusually bright (~1.0 crab) and relatively steady. The Fourier power density spectrum of the source was observed to vary with strong correlations among low-frequency flat-topped power (<~1--10 Hz), a quasi-periodic oscillation (QPO) peak centered at 1.3--12 Hz, and a broad QPO peak centered at ~20 Hz up to ~100 Hz. As orbital phase increased within the cycle, the rms amplitude of the flat-topped power generally (but not monotonically) decreased while the QPO features generally evolved toward higher frequency. The 1.5--12 keV spectrum was observed to generally harden during the nonflaring phases of each of the six 16.5 day periods monitored by the ASM.
Bradt Hale V.
Levine Alan M.
Morgan Edward Harrington
Shirey Robert E.
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