Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 171
... STARS Cool stars , in the temperature range 3000- 9000 K , emit most of their radiation in the wave- length range accessible from the ground ( as does our sun ) . However , as for the sun , the UV wavelength range reveals energetic ...
... STARS Cool stars , in the temperature range 3000- 9000 K , emit most of their radiation in the wave- length range accessible from the ground ( as does our sun ) . However , as for the sun , the UV wavelength range reveals energetic ...
Page 519
... stars , the masses of the components and the separations . Alterna- tively , the period of the binary and the evolu- tionary status of the components are useful , and we shall ... star was at one time the more massive one BINARY STARS 519.
... stars , the masses of the components and the separations . Alterna- tively , the period of the binary and the evolu- tionary status of the components are useful , and we shall ... star was at one time the more massive one BINARY STARS 519.
Page 521
... stars , al- though the mass ratio ranges from 0.1 to 1. Sur- face temperatures range from about 5500 to 8000 K. The lower mass systems are called W type , the higher mass ... Stars These systems are so named because of BINARY STARS 521.
... stars , al- though the mass ratio ranges from 0.1 to 1. Sur- face temperatures range from about 5500 to 8000 K. The lower mass systems are called W type , the higher mass ... Stars These systems are so named because of BINARY STARS 521.
Contents
Guide to Using the Encyclopedia ix Atomic Physics | 339 |
Approximations and Expansions 1 Atomic Spectrometry | 357 |
Archaeological Geology 31 Atomic Spectroscopy | 381 |
Copyright | |
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absorption acid aldoses angular momentum approximation asbestos atmosphere atoms auroral BASIC battery black hole Boolean algebra carbon fibers catalyst cell chemical chrysotile clouds collision complex components concentration convection cross section curve density developed disaccharide disk distribution dust electron elements emission emitted energy engine equations example expert system flux function galaxies heat hydrogen hydroxyl groups infrared input interaction interstellar interstellar medium ionization ions mass material measurements mechanism ment metal molecular molecules monosaccharides neutron stars nucleophile observed oligosaccharides operator orbital oxidation oxygen parameter particles photons plume problem radiation reaction reactor region result saccharide solar solution space spectral spectroscopy spectrum speed spline stable stars stellar structure surface techniques telescope temperature Theorem thermal tion tive turbulence ture typical variable velocity vertical wave wavelength weight white dwarf wind