THE MID-INFRARED APPEARANCE OF THE GALACTIC MINI-STARBURST W49A

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 50 young massive stars still enshrouded in their natal molecular cloud. We employ Spitzer/Infrared Spectrometer spectral mapping observations of the n...

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Bibliographic Details
Published in:The Astrophysical journal 2014-08, Vol.791 (2), p.1-20
Main Authors: Stock, D J, Peeters, E, Choi, W D-Y, Shannon, M J
Format: Article
Language:English
Subjects:
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Bands
COMPARATIVE EVALUATIONS
Continuums
Diffusion
EMISSION
Emission analysis
GIANT STARS
INFRARED SPECTROMETERS
INTERMEDIATE INFRARED RADIATION
MAGELLANIC CLOUDS
MAPPING
Massive stars
MILKY WAY
Polyallylamine hydrochloride
POLYCYCLIC AROMATIC HYDROCARBONS
Star formation
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Summary: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 50 young massive stars still enshrouded in their natal molecular cloud. We employ Spitzer/Infrared Spectrometer 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-H II (UC-H II) 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-H II regions-an effect previously observed only in one other object: the giant star forming region N66 in the Large Magellanic Cloud. 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-H II 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 H II regions.
ISSN:1538-4357
0004-637X
1538-4357
DOI:10.1088/0004-637X/791/2/99