Free Access

Fig. 3

image

Mid-IR spectra of IC 63 and IC 59 observed with the IRS instrument on board Spitzer. The spectra correspond to the SL and LL modules. For IC 63, we have chosen a 15′′ × 15′′ region at the tip of the nebula, along the second front seen in Fig. 4 where the PAH emission is the brightest. However, inspection of the entire data cube shows only small variations in the PAH band ratios throughout the tip of the nebula ( ≲40%). For IC 59, we took the average spectrum over a 25′′× 25′′ region at thetip of the nebula (see Fig. 2). Left panel: both spectra normalized to the peak intensity of the 11.3 μm feature (132.14 MJy sr−1 for IC 63 and9.34 MJy sr−1 for IC 59). Right panel: spectra normalized to the peak intensity of the 11.3 μm feature, after the subtraction of the continuum between 5 and 20 μm.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.