Bubbles, Bubbles Everywhere Bubbles

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Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..309c&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

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Scientific paper

The recent GLIMPSE mid-infrared imaging survey of the inner Galactic plane has revealed that dust bubbles pervade the Galactic disk. Here I summarize the projected spatial distribution of bubbles and their morphological properties (their size, shell thickness, and eccentricity distributions). The majority of the bubbles appear to be formed by young O and B stars. Analysis of their emission properties as a function of wavelength shows quite clearly that PAHs are destroyed inside the dust bubbles excited by O stars. However, dust is clearly observed to exist within the bubbles.

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