Add to ORKGBased on an improved model, more reasonable nucleosynthesis and explosion rate of SNeIa and CCSNe, we studied Mn evolution for three local dwarf spheroidal galaxies (dSphs), considering the detailed SNe yield and explosion rates for different types of progenitors. The results can explain the main observation of Mn abundance for tens stars in those dSphs, and give some constraints to the nucleosynthesis and explosion ratio of different types of supernovae and Star Formation Rates (SFR) in those dSphs
Recent extensive observations of Type Ia Supernovae (SNe Ia) have revealed the existence of a divers...
We model the evolution of manganese relative to iron in the progenitor system of the globular cluste...
We outline the results of a study of the chemical composition of 14 stars in the Sagittarius dwarf s...
The distribution of abundance for iron-peak elements in dwarf spheroidal galaxies (dSphs) is importa...
Manganese abundances are sensitive probes of the progenitors of Type Ia supernovae (SNe Ia). In this...
In our quest to identify the progenitors of Type Ia supernovae (SNe Ia), we first update the nucleos...
Aims. We model the chemical evolution of manganese relative to iron in three different stellar syst...
We provide manganese abundances (corrected for the effect of the hyperfine structure) for a large nu...
There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for...
We analyze the nucleosynthesis yields of various Type Ia supernova explosion simulations including p...
Context. Manganese is predominantly synthesised in Type Ia supernova (SN Ia) explosions. Owing to th...
Context. Manganese is an iron-peak element and although the nucleosynthesis path that leads to its f...
Context.Manganese is an iron-peak element and although the nucleosynthesis path that leads to its f...
Using three-dimensional hydrodynamical simulations of isolated dwarf spheroidal galaxies (dSphs), we...
There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for...
Recent extensive observations of Type Ia Supernovae (SNe Ia) have revealed the existence of a divers...
We model the evolution of manganese relative to iron in the progenitor system of the globular cluste...
We outline the results of a study of the chemical composition of 14 stars in the Sagittarius dwarf s...
The distribution of abundance for iron-peak elements in dwarf spheroidal galaxies (dSphs) is importa...
Manganese abundances are sensitive probes of the progenitors of Type Ia supernovae (SNe Ia). In this...
In our quest to identify the progenitors of Type Ia supernovae (SNe Ia), we first update the nucleos...
Aims. We model the chemical evolution of manganese relative to iron in three different stellar syst...
We provide manganese abundances (corrected for the effect of the hyperfine structure) for a large nu...
There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for...
We analyze the nucleosynthesis yields of various Type Ia supernova explosion simulations including p...
Context. Manganese is predominantly synthesised in Type Ia supernova (SN Ia) explosions. Owing to th...
Context. Manganese is an iron-peak element and although the nucleosynthesis path that leads to its f...
Context.Manganese is an iron-peak element and although the nucleosynthesis path that leads to its f...
Using three-dimensional hydrodynamical simulations of isolated dwarf spheroidal galaxies (dSphs), we...
There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for...
Recent extensive observations of Type Ia Supernovae (SNe Ia) have revealed the existence of a divers...
We model the evolution of manganese relative to iron in the progenitor system of the globular cluste...
We outline the results of a study of the chemical composition of 14 stars in the Sagittarius dwarf s...