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Generating Hot Gas in Simulations of Disk‐Galaxy Major Mergers

  • Authors: T. J. Cox, Joel Primack, Patrik Jonsson, and Rachel S. Somerville

Cox et al. 2004 The Astrophysical Journal Letters 607 L87.

  • Provider: AAS Journals

Caption: Fig. 2.

Remnant gas energy in units of keV per proton as measured 500 Myr after the merger between two disk galaxies plotted as a function of the orbital pericentric distance Rperi divided by the original disk scale length ﹩R_{d}﹩. Open circles are the progenitor disk galaxy 5 × MW, the largest progenitor disk galaxy; filled squares are MW disks; the asterisks are Dwarf1; and the filled triangles are Dwarf2. Solid lines are fits to the data using eq. (4) and described in the text.

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