| Issue |
A&A
Volume 504, Number 2, September III 2009
|
|
|---|---|---|
| Page(s) | 525 - 530 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/200912334 | |
| Published online | 16 July 2009 | |
Online Material
Table 3: V-band data used for examining the secular decrease in luminosity of the Crab Pulsar.
Table 4: UBVRIz magnitudes of the eight field stars examined in the secular decrease of luminosity of the pulsar.
![\begin{figure}
\par\includegraphics[width=10cm,clip]{12334fg4.eps}
\end{figure}](/articles/aa/olm/2009/35/aa12334-09/img87.png) |
Figure 4: The stars that were chosen for relative photometry in the investigation of the secular decrease in luminosity. The numbering is the same as in Table 4 where the UBVRIz magnitudes for these stars are given. The numbering is also used in Table 3. The pulsar is number eight. This V-band image was acquired with the JKT on February 7, 1990. North is up and east is to the left. The field of view is approximately 3.2 by 2.1 arcmin. |
| Open with DEXTER | |
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