Copy the page URI to the clipboard
Norton, A. J.; Somerscales, R. V. and Wynn, G. A.
(2004).
DOI: https://doi.org/10.1017/s0252921100002128
URL: http://www.aspbooks.org/a/volumes/table_of_content...
Abstract
We have used a model of magnetic accretion to investigate the rotational equilibria of magnetic cataclysmic variables (mCVs). This has enabled us toderive a set of equilibrium spin periods as a function of orbital period and magnetic moment which we use to estimate the magnetic moments of all known intermediate polars. We further show how these equilibrium spin periods relate to the polar synchronisation condition and use these results to calculate the theoretical histogram describing the distribution of magnetic CVs as a function of P_spin / P_orb. We demonstrate that this is in remarkable agreement with the observed distribution assuming that the number of systems as a function of white dwarf magnetic moment is distributed according to N(mu_1) ~ mu_1^-2.
Viewing alternatives
Download history
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from DimensionsItem Actions
Export
About
- Item ORO ID
- 4666
- Item Type
- Conference or Workshop Item
- ISBN
- 1-58381-170-2, 978-1-58381-170-2
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2004 Astronomical Society of the Pacific
- Depositing User
- Users 6042 not found.