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Understanding Stellar Evolution
, 2018Understanding Stellar Evolution is based on a series of graduate-level courses taught at the University of Washington since 2004. It describes the structure and evolution of stars, with emphasis on the basic physical principles and the interplay between ...
H. Lamers, E. Levesque
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The Structure and Evolution of Stars, 2019
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Rebecca Elliott
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Book file PDF easily for everyone and every device. You can download and read online Stellar Evolution file PDF Book only if you are registered here.
Rebecca Elliott
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Stellar Evolution and Stellar Structures
1995It is often thought that very little was known about the stars in the nineteenth century because most astronomy books of the time tended to concentrate on the planets. This was far from the truth, however, although nineteenth century knowledge of the stars was purely observational, with no understanding of their internal processes. In fact, at the time
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The STAROX stellar evolution code
Astrophysics and Space Science, 2007This paper describes the STAROX stellar evolution code for the calculation of the evolution of a model of a spherical star. The code calculates a model at time tk, that is the run of pressure, density, temperature, radius, energy flux and related variables on a mesh in mass Mi, given the distribution of chemical elements Xj(i) at tk and the model at ...
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La Rivista del Nuovo Cimento, 1971 Stellar Evolution and Stellar Populations in Galaxies
1992Models of population synthesis are resting on an ensemble of other models, data and assumptions, in particular the models of stellar evolution, the data on initial compositions, the data on stellar spectra, the initial mass function (IMF), the star formation rate (SFR), the infall rate, etc… Here we shall concentrate on the properties of stellar models
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STELLAR EVOLUTION AND PULSARS*
Annals of the New York Academy of Sciences, 1972It has been found that pulsars are rotating magnetic neutron stars, which are created during catastrophic collapses of old stars whose nuclear fuel has long since been used up. The maximum size of pulsars, based on the fastest rotation period of 33 msec, cannot exceed 100 km. The densest star the theory predicts is the neutron star.
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2012
We want to develop models of stellar evolution that can reproduce the mass–luminosity relation as well as the structure of the H-R diagram. Obviously, we will start with several simplifying assumptions that can be relaxed as we try to achieve better fidelity to observations.
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We want to develop models of stellar evolution that can reproduce the mass–luminosity relation as well as the structure of the H-R diagram. Obviously, we will start with several simplifying assumptions that can be relaxed as we try to achieve better fidelity to observations.
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Directed Evolution: Methodologies and Applications
Chemical Reviews, 2021Ye Li, Mingfeng Cao, Pu Xue
exaly