Abstract
An uninterrupted 62-hr observation of the nearby low luminosity type 1
Seyfert galaxy NGC4051 with the EXOSAT observatory is reported which
gives an order of magnitude improvement in the quality of the time
series and allows comparison with X-ray binaries. The observed power
spectral density is roughly proportional to 1/f, similar to Cyg X-1, and
characteristic of turbulent processes. No preferred timescale or
luminosity gradient has been seen so far. If this behavior holds
generally for active galactic nuclei, quantities derived from short
samples will be subject to selection effects.
Original language | English |
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Pages (from-to) | 694-696 |
Journal | Nature |
Volume | 325 |
Publication status | Published - 1 Feb 1987 |
Keywords
- Galactic Radiation
- Seyfert Galaxies
- Spaceborne Astronomy
- X Ray Astronomy
- Active Galactic Nuclei
- Exosat Satellite
- Light Curve
- Power Spectra
- Shot Noise