Astronomy & Astrophysics

$\begin{figure} \resizebox{8.9cm}{!}{\includegraphics*{avgenderenfig1.eps}}\end{figure}$ Figure 1: UBV ( $\bullet$ ) and BVR ( $\circ$ ) light curves of $\eta$ Car around the 2003.5 PP. Arrows below the V curve indicate the start of the declines in L and J, respectively. Star symbols: dates of X-ray flares. Arrows below the U curve: date X-ray decline, disappearance [NIII] line, start and end of X-ray totality.
Open with DEXTER

In the text

$\begin{figure} \resizebox{8.9cm}{!}{\includegraphics*{avgenderenfig2.eps}}\par\resizebox{8.9cm}{!}{\includegraphics*{avgenderenfig3.eps}}\end{figure}$ Figure 2: Top: light and colour curves ( $\bullet$ UBV, $\circ$ BVR). Vertical lines: start of X-ray decline, start and end of the X-ray totality. Bottom: V light curve ( $\bullet$ ) versus the 1998.0 y light curve (+) as shown in Fig. 2 of van Genderen et al. (2003). The y zeropoint has been shifted in order to match the V scale (y diaphragm is 22 $^{\prime \prime }$ ), the upper X-axis has been shifted by 5.5 yr.
Open with DEXTER

In the text

$\begin{figure} \resizebox{8.9cm}{!}{\includegraphics*{avgenderenfig1.eps}}\end{figure}$	Figure 1: UBV ( $\bullet$ ) and BVR ( $\circ$ ) light curves of $\eta$ Car around the 2003.5 PP. Arrows below the V curve indicate the start of the declines in L and J, respectively. Star symbols: dates of X-ray flares. Arrows below the U curve: date X-ray decline, disappearance [NIII] line, start and end of X-ray totality.
Open with DEXTER