Stellar Kinematics of Boxy Bulges: Large-Scale Bars and Inner Disks
(2004)
Formation and evolution of S0 galaxies: a SAURON case study of NGC7332
(2004)
A SAURON look at galaxy bulges
ASTRON NACHR 325:2 (2004) 92-95
Abstract:
Kinematic and population studies show that bulges are generally rotationally flattened systems similar to low-luminosity ellipticals. However, observations with state-of-the-art integral field spectrographs, such as SAURON, indicate that the situation is much more complex, and allow us to investigate phenomena such as triaxiality, kinematic decoupling and population substructure, and to study their connection to current formation and evolution scenarios for bulges of early-type galaxies. We present the examples of two SO bulges from galaxies in our sample of nearby galaxies: one that shows all the properties expected from classical bulges (NGC 5866), and another case that presents kinematic features appropriate for barred disk galaxies (NGC 7332).Bar-Driven Evolution and 2D Spectroscopy of Bulges
Chapter in Penetrating Bars through Masks of Cosmic Dust, Springer Nature 319 (2004) 139-148
HI and Hot Gas in the Outskirts of the M81 Group
Symposium - International Astronomical Union Cambridge University Press (CUP) 217 (2004) 452-457