![]() |
Figure 1a:
The ISO SWS spectrum of IRAS 14331-6435 (Hen3-1013)
shows emission due to amorphous (10.8 ![]() ![]() ![]() ![]() |
![]() |
Figure 1b:
The ISO SWS spectrum of IRAS 17311-4924 (Hen3-1428)
shows emission due to the UIR band at 7.7 ![]() ![]() ![]() ![]() ![]() |
![]() |
Figure 1c:
The ISO SWS spectrum of IRAS 22023+5249 (LSIII +5224)
shows emission due to amorphous (10.8 ![]() ![]() |
![]() |
Figure 2:
ISO SWS (2.4
![]() ![]() ![]() ![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 3:
Spectral energy distributions (SEDs) of the hot post-AGB stars.
![]() ![]() ![]() |
Open with DEXTER |
![]() |
Figure 3: continued. |
Open with DEXTER |