NGC 7023 at 3.3 μm
Date
A 3.3 μm polycyclic aromatic hydrocarbon (PAH) filter was used to study the photochemical evolution of PAHs in the reflection nebula NGC 7023. The filter is narrow, Δλ=0.09 μm, and isolates the PAH emission. The plate scale is 0.475 arcsec/pixel and the angular resolution is about 2 arcsec, dominated by telescope jitter. FORCAST also performed observations of NGC 7023 (at 11.2 μm) and the combined data shows a peak in the 11.2/3.3 μm ratio, corresponding to PAHs of ~50 C-atoms. This supports models claiming the photochemical evolution of PAHs is size-dependent and most efficient for PAHs with ~50 C-atoms.
Credit
Croiset et al. 2016, A&A, 590, A26.
Image Number
SCI2016_0007
Additional Information
NGC 7023 at 3.3 μm
Principal Investigator
B. A. Croiset
Instrument
FLITECAM
Location
United States
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