Image Details

Choose export citation format:

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. 5.

Computed population of cataclysmic variables at the current epoch in the M2Porb plane for our standard model (see Table 1). Here M2 is the mass of the donor star. The color represents the logarithm of the number of systems in a particular M2Porb cell, of which there are 100 per 0.1 M and 100 hr−1 interval in Porb. The color scale is given on the right‐hand side of the figure.

Other Images in This Article

Show More

Copyright and Terms & Conditions