SPH Simulations of the Chemical and Dynamical Evolution of the Galactic Bulge
1993 ◽
Vol 153
◽
pp. 395-396
Keyword(s):
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.
2022 ◽
2016 ◽
Vol 846
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pp. 73-78
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2012 ◽
Vol 09
(04)
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pp. 1250057
2007 ◽
Vol 375
(1)
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pp. 53-67
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2018 ◽
Vol 127
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pp. 47-58
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