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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. 10.

Computed distributions of the secondary (right‐hand panels) and white dwarf masses (left‐hand panels) in cataclysmic variables at the current epoch. The mass distributions are ordered according to the range of orbital period. The dotted histogram (upper right) is for post–period minimum CVs and has been arbitrarily divided by 1.5 for presentation purposes.

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