Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541404s&link_type=abstract
American Astronomical Society, AAS Meeting #215, #414.04; Bulletin of the American Astronomical Society, Vol. 42, p.254
Astronomy and Astrophysics
Astronomy
Scientific paper
We simulated characteristics of 2 bubbles, N28 and S146 in the mid-infrared spectrum, using Cloudy. The parameters for the 24μm best fit were: inner radius of 17.65 and a density of 1.06 (for N28), inner radius 18.01, and density 1.15 (for S146).When it came to fitting both the 24μm and 70μm fit, the data plot of the 70μm appeared above the 24μm, implying a cooler temperature, which in turn implied a larger grain distribution than that of the ISM or even the grain distribution found in the Orion nebula. The separation between the 70μm and 24μm simulated plot was not close to matching the data for the 70μm and 24μm plot. Even with the larger grain distribution we could not get a simulated plot to match the plot of the data.
Stafford Thomas
Watson Christer
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