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An Exploration of the Paradigm for the 2–3 Hour Period Gap in Cataclysmic Variables

  • Authors: Steve B. Howell, Lorne A. Nelson, and Saul Rappaport

Howell, Nelson, & Rappaport 2001 The Astrophysical Journal 550 897.

  • Provider: AAS Journals

Caption: Fig. 9.

Computed orbital period distributions for cataclysmic variables at the current epoch. Left panel: the solid curve is the distribution for all systems that appear in Fig. 3; the dashed curve was produced by scaling the contributions of each system evolved by ﹩\dot{M}^{3/ 2}﹩, while the dotted curve is for an ﹩\dot{M}^{1}﹩ scaling (see text). The ﹩\dot{M}^{3/ 2}﹩‐ and ﹩\dot{M}^{1}﹩‐scaled curves have been shifted vertically by arbitrary amounts for ease in comparison. Right panel: the solid curve is for all systems in Fig. 3 that have not yet reached orbital period minimum; the dashed curve is for systems that have evolved past the orbital period minimum.

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