The mid-infrared appearance of the Galactic Mini-Starburst W49A

Abstract

The massive star forming region W49A represents one of the largest complexes of massive star formation present in the Milky Way and contains at least fifty young massive stars still enshrouded in their natal molecular cloud. We employ Spitzer/IRS spectral mapping observations of the northern part of W49A to investigate the mid-infrared (MIR) spatial appearance of the polycyclic aromatic hydrocarbon (PAH) bands, PAH plateau features, atomic lines and continuum emission. We examine the spatial variations of the MIR emission components in slices through two of the ultra compact-HII (UC-HII) regions. We find that the PAH bands reproduce known trends, with the caveat that the 6.2 $\mu$m PAH band seems to decouple from the other ionized PAH bands in some of the UC-HII regions -- an effect previously observed only in one other object: the giant star forming region N66 in the LMC. Furthermore, we compare the nature of the emission surrounding W49A to that of `diffuse' sightlines. It is found that the surrounding emission can be explained by line of sight emission, and does not represent true `diffuse' material. Additionally, we examine the MIR appearance of star formation on various scales from UC-HII regions to starburst galaxies, including a discussion of the fraction of PAH emission in the 8 $\mu$m IRAC filter. We find that the MIR appearance of W49A is that of a starburst on large scales yet its individual components are consistent with other galactic HII regions.

23 pages, 14 figures, ApJ accepted

References in corpus (6)

• Mid-IR Galaxy Classification Based on Silicate Obscuration and PAH Equivalent Width
• Variations of the Mid-IR Aromatic Features Inside and Among Galaxies
• The Behavior of the Aromatic Features in M101 HII Regions: Evidence for Dust Processing
• Spectral Mapping Reconstruction of Extended Sources
• Spatially Resolved Spitzer-IRS Spectroscopy of the Central Region of M82
• The Mid-Infrared [SIV]/[NeII] versus [NeIII]/[NeII] Correlation

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• The 11.2 $\mu$m emission of PAHs in astrophysical objects
• Polycyclic Aromatic Hydrocarbon emission in Spitzer/IRS maps II: A direct link between band profiles and the radiation field strength
• Tracing PAH Size in Prominent Nearby Mid-Infrared Environments
• Characterizing the PAH Emission in the Orion Bar