<p>This is a software library for chemical evolution simulations of galaxy formation under the simple stellar population approximation. In this library, all of the necessary components concerning chemical evolution, such as initial mass functions, stellar lifetimes, yields from type II and Ia supernovae, asymptotic giant branch stars, and neutron star mergers, are compiled from the literature. Users can solve the evolution of 13 elements released from various events in their simulations via CELib APIs. </p> <p>This is CELib version 1.0.1. Please visit the bitbucket repository to obtain the latest version: https://bitbucket.org/tsaitoh/celib</p
Aims. Chemical evolution models are useful for understanding the formation and evolution of stars a...
Accepted for publication in Astrophysical JournalConsiglio Nazionale delle Ricerche (CNR). Bibliotec...
GALEV (GALaxy EVolution) evolutionary synthesis models describe the evolution of stellar populations...
One of the most important unsolved mysteries of astronomy is the formation and evolution of galaxies...
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
This thesis project involves the improvement of existing computer code, which is used in modeling th...
This thesis explores the chemical signatures of galaxy formation and evolution using a software pack...
Galaxies are complex systems where dynamics and chemical evolution are closely linked. In order to s...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
In this thesis we examine several improvements which can be made to the canonical under- standing of...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
Publisher's version/PDFWe present a new chemodynamical code – RAMSES-CH – for use in simulating the ...
We simulate the chemodynamical evolution of the Milky Way Galaxy, including the nucleosynthesis yiel...
The code CESAM is a consistent set of programs and routines which performs calculations of 1D quasi-...
Since stellar populations enhance particular element abundances according to the yields and lifetime...
Aims. Chemical evolution models are useful for understanding the formation and evolution of stars a...
Accepted for publication in Astrophysical JournalConsiglio Nazionale delle Ricerche (CNR). Bibliotec...
GALEV (GALaxy EVolution) evolutionary synthesis models describe the evolution of stellar populations...
One of the most important unsolved mysteries of astronomy is the formation and evolution of galaxies...
We have developed a new evolutionary synthesis code, which incorporates the output from chemical ev...
This thesis project involves the improvement of existing computer code, which is used in modeling th...
This thesis explores the chemical signatures of galaxy formation and evolution using a software pack...
Galaxies are complex systems where dynamics and chemical evolution are closely linked. In order to s...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
In this thesis we examine several improvements which can be made to the canonical under- standing of...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
Publisher's version/PDFWe present a new chemodynamical code – RAMSES-CH – for use in simulating the ...
We simulate the chemodynamical evolution of the Milky Way Galaxy, including the nucleosynthesis yiel...
The code CESAM is a consistent set of programs and routines which performs calculations of 1D quasi-...
Since stellar populations enhance particular element abundances according to the yields and lifetime...
Aims. Chemical evolution models are useful for understanding the formation and evolution of stars a...
Accepted for publication in Astrophysical JournalConsiglio Nazionale delle Ricerche (CNR). Bibliotec...
GALEV (GALaxy EVolution) evolutionary synthesis models describe the evolution of stellar populations...