... The stars and the ionized gas counterrotate over the whole FOV of the MPFS, and there is a hint of the reverse rotation for the stars at the edges of the SAURON FOV. ...
... stars with a radius of 5 -7 ; the bulge in which these "secondary" stellar ... stars in the bulge, the star-formation burst at the center of IC 1548 initially ... stars) NGC 83 (stars) NGC 83 (gas) NGC 93 (stars) NGC 79 (stars) NGC 86 (stars) IC ...
... star formation in NGC 516 lasted longer than that in the center of NGC 509, that the ... burst of star formation in the nucleus and a subsequent continuous process of star ...
... stars by crosscorrelating in dividual spectra with spectra of bright K giant stars ... stars and ionized gas in the center of NGC 759 Fig. 7 presents isovelocity maps for ...
... star-formation burst in it but simply suggests that the secondary star formation ... STARS IN THE CENTRAL REGION OF NGC 4548 In kinematic studies, the use of two ... stars is also oriented at PA0,kin = 145 , this coincidence proves that the rotation ...
... star formation ring being elliptical in the galactic plane: both observations (Buta ... star formation may be just tilted to the galactic plane and rotates together with ...
... star velocities and stellar velocity dispersions are calculated by cross-correlating ... STAR FORMATION IN THE CENTERS OF NGC 3599 AND NGC 3626 The Lick index system is well ...
... However, this is the same process that leads to the gradual establishment of an exponential star surface density profile if the stars are formed on the time scales of the radial redistribution of gas (Lin and Pringle 1987)! ...
... star formation process stops between these two moments, the stars would have a ... star formation within it had to be strongly inhomogeneous, with an exotic mechanism ...