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The Probability Distribution Function of Gas Surface Density in M33
Edvige Corbelli, Bruce G. Elmegreen, Jonathan Braine +1
The probability distribution functions (PDFs) for atomic, molecular, and total gas surface densities of M33 are determined at a resolution of about 50~pc over regions that share co…
Simulations of the flocculent spiral M33: what drives the spiral structure?
C. L. Dobbs, A. R. Pettitt, E. Corbelli +1
We perform simulations of isolated galaxies in order to investigate the likely origin of the spiral structure in M33. In our models, we find that gravitational instabilities in the…
Properties and rotation of molecular clouds in M 33
Jonathan Braine, Erik Rosolowsky, Pierre Gratier +2
The sample of 566 molecular clouds identified in the CO(2--1) IRAM survey covering the disk of M~33 is explored in detail.The clouds were found using CPROPS and were subsequently c…