会议专题

X-ray timing studies of Active Galactic Nuclei

We present a power spectral analysis survey of 24 active galactic nuclei (AGN). We combine x-ray observations to produce a power spectrum covering a broad range of Fourier frequencies and fit the power spectrum of each AGN using a single-bend power-law model. Using the resultant bend time-scales of 18 AGN, and of the Galactic black hole X-ray binaries Cyg X-1 and GRS1915+105, We present a plot of observed bend time-scales versus the predicted bend time-scales determined from published masses and bolometric luminosities. The results confirm our previously proposed scaling relation of bend time- scale with mass divided by accretion rate. All work

galaxies active-galaxies Seyfert-X rays galaxies

D. P Summons I. M. McHardy P. Uttley P. Arevalo A. Bhaskar

School of Physics and Astronomy, University of Southampton, Southampton, Hampshire, SO17 1BJ, UK Sch School of Physics and Astronomy, University of Southampton, Southampton, Hampshire, SO17 1BJ, UK School of Engineering Science, University of Southampton, Southampton, Hampshire, SO17 1BJ, UK

国际会议

紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)

安徽黄山

英文

381-383

2007-07-01(万方平台首次上网日期,不代表论文的发表时间)