2011A&A...532A.128R


C.D.S. - SIMBAD4 rel 1.7 - 2020.08.09CEST13:24:03

2011A&A...532A.128R - Astronomy and Astrophysics, volume 532A, 128-128 (2011/8-1)

Coupled blind signal separation and spectroscopic database fitting of the mid infrared PAH features.

ROSENBERG M.J.F., BERNE O., BOERSMA C., ALLAMANDOLA L.J. and TIELENS A.G.G.M.

Abstract (from CDS):

The aromatic infrared bands (AIBs) observed in the mid infrared spectrum of galactic and extragalactic sources are attributed to polycyclic aromatic hydrocarbons (PAHs). Recently, two new approaches have been developed to analyze the variations of AIBs in terms of chemical evolution of PAH species: blind signal separation (BSS) and the NASA Ames PAH IR Spectroscopic Database fitting tool. We aim to study AIBs in a photo-dissociation region (PDR) since in these regions, as the radiation environment changes, the evolution of AIBs are observed. We observe the NGC 7023-north west (NW) PDR in the mid-infrared (10-19.5µm) using the InfraRed Spectrometer (IRS), on board Spitzer, in the high-resolution, short wavelength mode. Clear variations are observed in the spectra, most notably the ratio of the 11.0 to 11.2µm bands, the peak position of the 11.2 and 12.0µm bands, and the degree of asymmetry of the 11.2µm 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 PAH+ and PAH0 and provides confidence in both methods for producing reliable results. The 11.0µm feature is attributed to PAH+ while the 11.2µm band is attributed to PAH0. The VSG signal shows a characteristically asymmetric broad feature at 11.3µm 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.

Abstract Copyright:

Journal keyword(s): astrochemistry - photon-dominated region (PDR) - ISM: lines and bands - infrared: ISM

Errata: corrigendum vol.537, art. C5 (2012)

Simbad objects: 3

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Number of rows : 3

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1485 0
2 NGC 7023 RNe 21 01 36.9 +68 09 48           ~ 631 0
3 HD 200775 Ae* 21 01 36.9184805541 +68 09 47.770037306 7.34 7.754 7.427 8.13   B2Ve 509 0

    Equat.    Gal    SGal    Ecl

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2020.08.09-13:24:03

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