X-ray emission from intermediate polars and open clusters
We have implemented a full 3-dimensional model to generate the X-ray lightcurves and spectra of intermediate polars using the traditional accretion curtain model as a basis. The model constitutes an improvement over previous works because it includes the effects of tall, structured accretion columns...
Main Author: | |
---|---|
Published: |
Keele University
2003
|
Subjects: | |
Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.397516 |