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Results 1 - 10
of
1,021
Galactic and Cosmic Chemical Evolution
, 2005
"... Abstract. We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss the ..."
Abstract
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Abstract. We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss
Galactic and Cosmic Chemical Evolution
, 2005
"... Abstract. We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss the ..."
Abstract
- Add to MetaCart
Abstract. We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss
Galactic chemical evolution: Carbon through Zinc
, 2006
"... We calculate the evolution of heavy element abundances from C to Zn in the solar neighborhood adopting our new nucleosynthesis yields. Our yields are calculated for wide ranges of metallicity (Z = 0 − Z⊙) and the explosion energy (normal supernovae and hypernovae), based on the light curve and spect ..."
Abstract
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We calculate the evolution of heavy element abundances from C to Zn in the solar neighborhood adopting our new nucleosynthesis yields. Our yields are calculated for wide ranges of metallicity (Z = 0 − Z⊙) and the explosion energy (normal supernovae and hypernovae), based on the light curve
AN INTRODUCTION TO GALACTIC CHEMICAL EVOLUTION
, 709
"... Abstract. The formalism of the simple model of galactic chemical evolution (GCE) and its main ingredients (stellar properties, initial mass ..."
Abstract
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Abstract. The formalism of the simple model of galactic chemical evolution (GCE) and its main ingredients (stellar properties, initial mass
PN and galactic chemical evolution
, 2001
"... Abstract. Recent applications of PN to the study of galactic chemical evolution are reviewed, such as PN and stellar populations, abundance gradients, including their space and time variations, determination of the He/H radial gradient and of the helium-to-metals enrichment ratio, and the [O/Fe] × ..."
Abstract
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Abstract. Recent applications of PN to the study of galactic chemical evolution are reviewed, such as PN and stellar populations, abundance gradients, including their space and time variations, determination of the He/H radial gradient and of the helium-to-metals enrichment ratio, and the [O
Galactic Chemical Evolution
, 2003
"... The primary present-day observables upon which theories of galaxy evolution are based are a system’s morphology, dynamics, colour, and chemistry. Individually, each provides an important constraint to any given model; in concert, the four represent a fundamental (intractable) boundary condition for ..."
Abstract
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Cited by 2 (0 self)
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The primary present-day observables upon which theories of galaxy evolution are based are a system’s morphology, dynamics, colour, and chemistry. Individually, each provides an important constraint to any given model; in concert, the four represent a fundamental (intractable) boundary condition
galactic chemical evolution
, 2002
"... Dispersal of massive star products and consequences for ..."
Results 1 - 10
of
1,021
