β Scribed by V. S. Shorin; V. M. Gribunin; V. N. Kononov; I. I. Sidorova
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
We present new results of the nucleosynthesis of s-elements in hot AGB stars. In the framework of the overshoot model, we show that the s-process nucleosynthesis depends sensitively on the thermodynamical conditions of the mixing zone and depending on the stellar mass and unknown overshoot parameter
Enhanced deuterium was not detected in the metal-poor halo stars HD 140283, the protoplanetary nebula AFGL 2688, or the Orion nebula. The Galactic Center (GC) deuterium abundance in the 50 km/s molecular cloud is (2.0-10)Γ 10 -6 and less than the local ISM D/H = (0.9-1.7)x10 -5. Thus the GC D result
For the astrophysical p process a complex reaction network has to be solved. In the order of 10,000 theoretically predicted reaction rates are needed for simulations of this network. For reactions involving Ξ± particles or protons, the predictions in the framework of the Hauser-Feshbach (HF) model w