Results 351 to 360 of about 1,652,070 (380)
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How Massive Single Stars End Their Life
, 2002How massive stars die—what sort of explosion and remnant each produces—depends chiefly on the masses of their helium cores and hydrogen envelopes at death.
A. Heger +4 more
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Mathematical Proceedings of the Cambridge Philosophical Society, 1939
Difficulties associated with the evolution of stars by radiation alone are briefly discussed. It is clear that some other process is also affecting the stars and it is shown that the stars are capable of adding to their mass by the process of accretion of the cosmical cloud.
R. A. Lyttleton, Fred Hoyle
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Difficulties associated with the evolution of stars by radiation alone are briefly discussed. It is clear that some other process is also affecting the stars and it is shown that the stars are capable of adding to their mass by the process of accretion of the cosmical cloud.
R. A. Lyttleton, Fred Hoyle
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2017
In cinema, theParisienne type is often overdetermined by the star incarnating the role, pointing to more extra-cinematic considerations in the construction of la Parisienne in cinema. Certain actors possess a Parisienne iconographical profile which develops out of intra-, inter-, and extra-cinematic considerations.
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In cinema, theParisienne type is often overdetermined by the star incarnating the role, pointing to more extra-cinematic considerations in the construction of la Parisienne in cinema. Certain actors possess a Parisienne iconographical profile which develops out of intra-, inter-, and extra-cinematic considerations.
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Interdisciplinary Science Reviews, 1987
AbstractThe Strategic Defense Initiative, SDI, commonly called Star Wars, is here critically analysed. The almost inconceivable destruction caused by nuclear war and the following nuclear winter are described, along with the various difficulties of intercepting Intercontinental Ballistic Missiles, ICBMS, are discussed in technical detail.
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AbstractThe Strategic Defense Initiative, SDI, commonly called Star Wars, is here critically analysed. The almost inconceivable destruction caused by nuclear war and the following nuclear winter are described, along with the various difficulties of intercepting Intercontinental Ballistic Missiles, ICBMS, are discussed in technical detail.
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Stars that Shimmer and Stars that Shine
2017Stars are not only much higher performing than their peers, but also much more visible within the firm. Star employees are likely to be sought out by their lower-performing peers. Moreover, high visibility and frequent interaction make it likely that the stars will develop abundant social capital.
Shad S. Morris, James B. Oldroyd
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1987
Normal stars G-type stars are characterized by weak hydrogen lines which become comparable in strength to the lines of some metals. Metallic lines increase both in number and in intensity toward later spectral subdivisions, and molecular bands of CH and CN become easily visible features.
Carlos Jaschek, Mercedes Jaschek
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Normal stars G-type stars are characterized by weak hydrogen lines which become comparable in strength to the lines of some metals. Metallic lines increase both in number and in intensity toward later spectral subdivisions, and molecular bands of CH and CN become easily visible features.
Carlos Jaschek, Mercedes Jaschek
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Black Holes, White Dwarfs, and Neutron Stars
, 1983S. Shapiro, S. Teukolsky
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Star Products, Star Exponentials, and Star Functions
2018We give a brief review on non-formal star products and star exponentials and star functions (Omori et al., Deformation of expressions for elements of an algebra, in Symplectic, Poisson, and Noncommutative Geometry. Mathematical Sciences Research Institute Publications, vol. 62 (Cambridge University Press, Cambridge, 2014), pp.
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Habitable zones around main sequence stars.
Icarus (New York, N.Y. 1962), 1993J. Kasting, D. Whitmire, R. Reynolds
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