Eclipse mapping of accretion discs
Abstract
The eclipse mapping method is an inversion technique that makes use of the information contained in eclipse light curves to probe the structure, the spectrum and the time evolution of accretion discs. In this review I present the basics of the method and discuss its different implementations. I summarize the most important results obtained to date and discuss how they have helped to improve our understanding of accretion physics, from testing the theoretical radial brightness temperature distribution and measuring mass accretion rates to showing the evolution of the structure of a dwarf novae disc through its outburst cycle, from isolating the spectrum of a disc wind to revealing the geometry of disc spiral shocks. I end with an outline of the future prospects.
Keywords
Cite
@article{arxiv.astro-ph/0009472,
title = {Eclipse mapping of accretion discs},
author = {Raymundo Baptista},
journal= {arXiv preprint arXiv:astro-ph/0009472},
year = {2007}
}
Comments
19 pages, 13 figures, to appear in the proceedings of the Astro-Tomography workshop, eds. H. Boffin & D. Steeghs, Springer-Verlag Lecture Notes in Physics