An Introduction to the Theory of Stellar Structure and Evolution

By D. Prialnik. 2000

298 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/368e4f728efae61b1dfa9aafce2f2598b4aa3b88

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. Santi Cassisi
2. Maurizio Salaris
3. Aomawa L. Shields
4. S. Ballard
5. J. Johnson
6. A. Milone
7. Timothy Morton
8. G. Piotto

Citations in the corpus

• Evolution of Stars and Stellar Populations (2005, background): “[115], [155]) that in a thin shell of thickness s, located at a radial coordinate r, pressure and density changes are related through:”
• The Habitability of Planets Orbiting M-dwarf Stars (2016, background): “Bacteria can increase their osmotic pressure in response to dry conditions (Yancey et al., 1982), allowing water to flow from areas of low solute concentration to high solute concentration, protecting the cytoplasm (cell interior) from dehydration, and stabilizing proteins (Potts, 1994).”