![\begin{figure}
\par\includegraphics[width=16.9cm,height=15.1cm,clip]{mainfig.eps}\end{figure}](/articles/aa/full/2004/46/aa0315-04/Timg24.gif) |
Figure 1:
Spectral energy distributions of 6 FU Orionis-type
objects. Open symbols correspond to the epoch of 1983 while
filled symbols mark the SED as of 1996-2000. The data are presented
with no reddening correction. Error bars smaller than the symbol size
were not plotted. For V1331 Cyg there are no NIR data from 1983; we
plotted data from 1979 (the K-band lightcurve shows constant flux in
this period). In the case of V346 Nor the ISO and IRAS beams also
include the nearby pre-main sequence star Reipurth 13. For comparison the
plotted MSX flux densities are sums of the individual fluxes of the
two objects. |