Modeling CO emission from hydrodynamic simulations of nearby spirals, starbursting mergers, and high-redshift galaxies

F. Bournaud; E. Daddi; A. Weiß; F. Renaud; C. Mastropietro; R. Teyssier

doi:10.1051/0004-6361/201425078

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Volume 575 (March 2015)

A&A, 575 (2015) A56

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Fig. 9

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Phase-space distribution of the ISM in a high-z disk snapshot (black) and its giant clumps (green), selected as in Figs. 3 and 4. The figure shows the density-temperature space, with isodensity contours encompassing 90% of the total gas mass (solid) and 67% of the total gas mass (dashed).

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