Orbital structure of triaxial galaxies
IAU SYMP (2004) 179-180
Abstract:
We have developed a method to construct realistic triaxial dynamical models for elliptical galaxies, allowing us to derive best-fitting parameters, such as the mass-to-light ratio and the black hole mass, and to study the orbital structure. We use triaxial theoretical Abel models to investigate the robustness of the method.Parametric recovery of line-of-sight velocity distributions from absorption-line spectra of galaxies via penalized likelihood
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 116:816 (2004) 138-147
Probing the dark ages with the Square Kilometer Array
NEW ASTRONOMY REVIEWS 48:11-12 (2004) 1029-1038
Rotating Halos and Heavy Disks: the Case of NGC 2915
Symposium - International Astronomical Union Cambridge University Press (CUP) 217 (2004) 172-173
Rotating Halos and Heavy Disks: The Case of NGC 2915
Symposium - International Astronomical Union Cambridge University Press (CUP) 220 (2004) 293-298