Montage Used In Study Of Polycyclic Aromatic Hydrocarbons (PAHs)

Rosenberg et al. (2011) recently reported on a study of Polycyclic Aromatic Hydrocarbons(PAHS), which cause very strong emission line features in the mid-infrared (10 – 20 microns), in the Photo-Dissociation Region (PDR) of  NGC 7023. As part of this study, they obtained Spitzer observations of the PAH’s, and used Montage to regrid maps of the power in the emission lines as a starting point for their analysis.

IRAC 8 micron image of NGC 7023. The white box is the field of study around the PDR NGC 7023-NW.

IRAC 8 micron image of NGC 7023. The white box is the field of study around the PDR NGC 7023-NW.

Rosenberg et al. write:  “The aromatic infrared bands (AIBs) observed in the mid infrared spectrum are attributed to Polycyclic Aromatic Hydrocarbons (PAHs). We observe the NGC 7023-North West (NW) PDR in the mid-infrared (10 – 19.5 micron) using the Infrared Spectrometer (IRS), on board Spitzer. Clear variations are observed in the spectra, most notably the ratio of the 11.0 to 11.2 micron bands, the peak position of the 11.2 and 12.0 micron bands, and the degree of asymmetry of the 11.2 micron band. The observed variations appear to change as a function of position within the PDR. We aim to explain these variations by a change in the abundances of the emitting components of the PDR. A Blind Signal Separation (BSS) method, i.e. a Non-Negative Matrix Factorization algorithm is applied to separate the observed spectrum into components. Using the NASA Ames PAH IR Spectroscopic Database, these extracted signals are fit. The observed signals alone were also fit using the database and these components are compared to the BSS components. Three component signals were extracted from the observation using BSS. We attribute the three signals to ionized PAHs, neutral PAHs, and Very Small Grains (VSGs). The fit of the BSS extracted spectra with the PAH database further confirms the attribution to ionized and neutral PAHs and provides confidence in both methods for producing reliable results. The 11.0 micron feature is attributed to PAH cations while the 11.2 micron band is attributed to neutral PAHs. The VSG signal shows a characteristically asymmetric broad feature at 11.3 micron with an extended red wing. By combining the NASA Ames PAH IR Spectroscopic Database fit with the BSS method, the independent results of each method can be confirmed and some limitations of each method are overcome.”

This entry was posted in astronomy, astronomy images, Astronomy software, Image mosaic, Image processing, Images, software, Software engineering and tagged , , , , , . Bookmark the permalink.

Leave a Reply

Fill in your details below or click an icon to log in: Logo

You are commenting using your account. Log Out /  Change )

Google+ photo

You are commenting using your Google+ account. Log Out /  Change )

Twitter picture

You are commenting using your Twitter account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )


Connecting to %s