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Uncovering the integral spectral characteristics of the planetary nebula IC 4642. [PDF]
Sci RepMohery M +4 more
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A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
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2004
Abstract The physical structures and properties of stars change as they age. In this chapter, we give an overview of the way stars evolve to set the context for our later discussions. The mass is by far the most important single factor determining a star’s structure and evolution.
T W Hartquist, J E Dyson, D P Ruffle
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Abstract The physical structures and properties of stars change as they age. In this chapter, we give an overview of the way stars evolve to set the context for our later discussions. The mass is by far the most important single factor determining a star’s structure and evolution.
T W Hartquist, J E Dyson, D P Ruffle
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Fred’s Contributions to Stellar Evolution
Astrophysics and Space Science, 2003zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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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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Stellar Populations, Stellar Evolution, and Stellar Atmospheres
2021J. J. Eldridge, E. R. Stanway
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