Doppler Tomography
Doppler Tomography is a scholarly work, published in 2005 in ''Astrophysics and Space Science''. The main subjects of the publication include astrophysics, gamma-ray burst, tomographic reconstruction, astronomy, Doppler imaging, Stars, accretion, quantum orbital motion, Doppler effect, binary star, line, binary numeral system, orbital plane, star formation, tomography, and physics. Author review the method of Doppler tomography which is widely used to understand the complex emission line profile variations displayed by accreting binary stars.