Abstract
The Seyfert galaxy NGC4151 was observed continuously in bands V and K
for several hours each night during the week 1979 May 14-21. In our 22
arcsec aperture its magnitude remained constant to better than 0.05 mag
at V = 12.01 and K = 8.67 on all time-scales from minutes to one week.
The implications of differing characteristic time-scales of variability
in different wavebands for the structure of the nucleus are discussed.
Original language | English |
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Pages (from-to) | 149-154 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 195 |
DOIs | |
Publication status | Published - 1 Apr 1981 |
Keywords / Materials (for Non-textual outputs)
- Galactic Nuclei
- Galactic Structure
- Infrared Astronomy
- Seyfert Galaxies
- Visual Photometry
- Calibrating
- Variability
- X Ray Astronomy