![\begin{figure}
\par\includegraphics[angle=-90,width=8.8cm,clip]{Fi291_f1.eps}
\end{figure}](/articles/aa/full/2004/05/aafi291/img25.gif) |
Figure 1:
The spectra show, from bottom to top, the KIII template
(with lines multiplied by 0.14), the average Doppler-corrected spectrum of GRS 1915+105 (16
spectra), the difference spectrum (thus, representing the disk
spectrum) and the difference spectrum between the template and the
average Doppler-corrected spectrum of GRS1915+105 at binary phase
 0.75 (the same average spectrum as in Greiner et al. 2001b). |
| Open with DEXTER | |
In the text