In this paper we present an objective map of the cyclotron emission region in a magnetic cataclysmic variable from polarimetric observations of the AM Her system V347 Pav. As the system parameters of V347 Pav (for example its inclination) have not been well determined, we describe an extension to Stokes imaging of Paper I which also searches the system parameter space.
No takes yet. Share an insight, caveat, or question.
Potter et al. (2000) studied this question.
Synapse has enriched one closely related paper. Consider it for comparative context: