![\begin{figure}
\par\resizebox{8.8cm}{!}{\includegraphics[angle=270,clip]{Fk114f1.ps}}
\end{figure}](/articles/aa/full/2004/02/aafk114/img19.gif) |
Figure 1:
Left panel: H
profile obtained with UVES (21/9/2003) -
note the narrow (
 km s-1) double peaked profile (
 km s-1, central
absorption blueshifted 31 km s-1 from rest wavelength)
and emission wings extending to projected
velocities of  103 km s-1. Right panel: Comparison of blended profiles
of Pa11 and N I 8747 Å from the NTT (2003 June 7; red dotted lines)
and the VLT (2003 September 21; solid black lines, resolution degraded to match the
NTT spectrum) demonstrating continued spectral evolution over only 3 months. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\resizebox{8.8cm}{!}{\includegraphics[angle=270,clip]{Fk114f2.ps}}
\end{figure}](/articles/aa/full/2004/02/aafk114/img20.gif) |
Figure 2:
Narrow (
 km s-1), single peaked profiles of
He I 6678 Å (left panel;
 Å) and 7065 Å (right panel;
 Å)
from UVES data (rest wavelengths indicated). |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\resizebox{18cm}{!}{\includegraphics[angle=270,clip]{Fk114f3.ps}}
\end{figure}](/articles/aa/full/2004/02/aafk114/img22.gif) |
Figure 3:
I band (8200-9000 Å) spectra of W243 obtained
between 2002-2003 compared to spectra of B & A supergiant standards (data from Munari & Tomasella
1999).
Note the overlap in wavelength ranges betwen upper
and lower panels. Principal transitions are indicated; the broad
absorption feature at  8620 Å is a DIB and is common to all our spectra of Wd 1 members.
The spectrum of the peculiar YHG IRC+10 420 is also presented; a
wavelength shift has been applied to this spectrum to correct for the
systemic
and intrinsic velocity shifts identified for this object by Oudmaijer
(1998). |
| Open with DEXTER | |
In the text