scholarly journals Angular momentum transport and disc morphology in smoothed particle hydrodynamics simulations of galaxy formation

2007 ◽  
Vol 375 (1) ◽  
pp. 53-67 ◽  
Author(s):  
T. Kaufmann ◽  
L. Mayer ◽  
J. Wadsley ◽  
J. Stadel ◽  
B. Moore
1993 ◽  
Vol 153 ◽  
pp. 395-396
Author(s):  
T. Tsujimoto ◽  
K. Nomoto ◽  
T. Shigeyama ◽  
Y. Ishimaru

We simulate the chemical and dynamical evolution of the galactic bulge with the smoothed particle hydrodynamics (SPH) method. We calculate the early phase of galaxy formation in which the bulge is formed through a burst of star formation. The calculated abundance distribution function of stars in the bulge is consistent with the observations of bulge K giants, if the heavy element yields are three times larger than those expected from Salpeter's IMF.


2010 ◽  
Vol 408 (2) ◽  
pp. 812-826 ◽  
Author(s):  
G. S. Stinson ◽  
J. Bailin ◽  
H. Couchman ◽  
J. Wadsley ◽  
S. Shen ◽  
...  

2001 ◽  
Vol 320 (2) ◽  
pp. 261-280 ◽  
Author(s):  
A. J. Benson ◽  
F. R. Pearce ◽  
C. S. Frenk ◽  
C. M. Baugh ◽  
A. Jenkins

2008 ◽  
Vol 96 (6) ◽  
pp. 263-268 ◽  
Author(s):  
E. Mounif ◽  
V. Bellenger ◽  
A. Ammar ◽  
R. Ata ◽  
P. Mazabraud ◽  
...  

2020 ◽  
Vol 59 (40) ◽  
pp. 18236-18246
Author(s):  
Tianwen Dong ◽  
Yadong He ◽  
Jianchun Wu ◽  
Shiyu Jiang ◽  
Xingyuan Huang ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document