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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. 2.

Evolution with orbital period, Porb, of the mass transfer rate, ﹩\dot{M}﹩, secondary mass, M2, and secondary radius, R2, for several illustrative model cataclysmic variable systems. The initial masses for the systems whose evolutions are displayed in the left and right sets of panels are the same as described in Fig. 1.

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