Abstract
Long-term monitoring of the X-ray source associated with the nucleus of
NGC 5128 has produced the most complete light curve in any frequency
band for this peculiar active galaxy. The X-ray data indicate activity
on at least two time scales: (1) a slow outburst with a time scale of
4-7 yr, (2) superimposed flares with a time scale of 20-50 day. This
pattern of behavior is related to other X-ray active galaxies:
specifically NGC 4151 (Seyfert) and MKN 421 (BL Lac). Some similarities
are noted.
| Original language | English |
|---|---|
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 181 |
| DOIs | |
| Publication status | Published - 1 Dec 1977 |
Keywords / Materials (for Non-textual outputs)
- Ariel Satellites
- Black Holes (Astronomy)
- Galactic Nuclei
- Light Curve
- Sky Surveys (Astronomy)
- X Ray Sources
- Active Galaxies
- Centaurus Constellation
- Frequencies
- Galactic Radiation
- Peculiar Galaxies
- Radiant Flux Density
- Radioactivity
- Seyfert Galaxies
- Spectral Bands
- Time
- Variability
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