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
SAURON dynamical modeling of NGC 2974
IAU SYMP (2004) 305-306
Abstract:
We present a three-integral orbit superposition Schwarschild model of NGC 2974, observed with the integral-field unit SAURON. We explore the dynamical structure of the stars and gas.SPIFFI observations of the starburst SMM J14011+0252: Already old, fat, and rich by z=2.565
ASTROPHYSICAL JOURNAL 605:2 (2004) 109-112
The 2dF Galaxy Redshift Survey: spherical harmonics analysis of fluctuations in the final catalogue
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 353:4 (2004) 1201-1218