Titlebook: Astrotomography; Indirect Imaging Met Henri M.J. Boffin,Jan Cuypers,Danny Steeghs Book 2001 Springer-Verlag Berlin Heidelberg 2001 Accretio

hankering

The Method of Spectra Disentangling and Its Links to Doppler Tomography,ial velocities for known component spectra - was best solved by the cross-correlation technique. The method of Fourier disentangling solves simultaneously both parts of this problem in a very effective way. It is shown here that its principle can also be used for Doppler tomography.

syncope

有偏見

David Gibson,Kathryn Coleman,Leah Irvingsting that it forms in a high electron density region. This again favours the idea that the central spike originates in the white dwarf. We present Doppler maps obtained for the emission lines which show three clear emission regions.

柔美流暢

Ganglion-Cyst

Midfacial Aging – Deflation or Descent?e recovered with good accuracy, even if the phase coverage per rotation cycle is poor, provided the total data set is long enough. From observations of the HR 1099 K1 subgiant secured in 1998, 1999 and 2000, we obtain that the equator rotates faster than the pole with a rotational shear about 3 times smaller than solar.