Turbulence within dust clouds (TB). Good Afternoon. Quendella Taylor Northern Arizona University/Penn State. Turbulence within dust clouds (TB).
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Why should we study ‘TB’? Because turbulence may answers many of the fundamental questions . For example what conditions are desirable for star formation to occur, what happens in the vicinity of star forming areas, IMF ,etc.In addition we are developing tools in order to study diffuse emission, in the GLIMPSE survey regions.
How can we study ‘TB’? By using the structure function SF(l) and the power spectrum P(k) to analyze images taken from 2mass and MSX .
What are the SF(l) and P(k)? They are tools we are going to use in order to understand ‘TB’. By removing the stars from images we may be able to isolate the diffuse emission .