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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. 4.

Computed population of cataclysmic variables at the current epoch in the ﹩R_{2}- P_{\mathrm{orb}\,}﹩ plane for our standard model (see Table 1). Here R2 is the radius of the donor star. The color represents the logarithm of the number of systems in a particular R2Porb cell, of which there are 100 per 0.1 R and 100 per hour interval in Porb. The color scale is given on the right‐hand side of the figure.

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