Dynamical Modeling of SAURON Galaxies (CROSBI ID 506479)
Prilog sa skupa u zborniku | sažetak izlaganja sa skupa | međunarodna recenzija
Podaci o odgovornosti
Cappellari, M. ; van den Bosch, R. C. E. ; Verolme, E. K. ; Bacon, R. ; Bureau, M. ; Copin, Y. ; Davies, R. L. ; Emsellem, E. ; Krajnović, Davor ; Kuntschner, H. ; and 4 coauthors
engleski
Dynamical Modeling of SAURON Galaxies
We describe our program for the dynamical modeling of early-type galaxies obs erved with the panoramic integral-field spectrograph SAURON. We are using Schwar zschild's numerical orbit superposition method to reproduce in detail all kinema tical and photometric observables, and recover the intrinsic orbital structure o f the galaxies. Since catastrophes are the most prominent features in the orbita l observables, two-dimensional kinematical coverage is essential to constrain th e dynamical models.
Galaxies: Elliptical and Lenticular; Galaxies: Kinematics and Dynamics
Nepotpun bibliografski opis - nedostaje broj stranica.
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Podaci o prilogu
2003.
objavljeno
Podaci o matičnoj publikaciji
Carnegie Observatories Astrophysics Series, Vol. 1: Coevolution of Black Holes and Galaxies
Ho, L. C.
Pasadena (CA): Carnegie Observatories
Podaci o skupu
Coevolution of Black Holes and Galaxies
predavanje
02.02.2003-05.02.2003
Pasadena (CA), Sjedinjene Američke Države
