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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. 7.

Computed population of cataclysmic variables at the current epoch in the Teff /Porb plane (left panel) and the luminosity‐Porb plane (right panel) for our standard model (see Table 1). We show both the stellar luminosity (top curve) and the core nuclear luminosity (lower distributions). The color represents the logarithm of the number of systems in a particular LPorb or TeffPorb cell, of which there are 100 per decade in L, 100 per 500 K in Teff, and 100 per hour interval in Porb. The color scale for both plots is given on the right‐hand side of the figure.

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