Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 191
... becoming much smaller . If their final mass is small enough , they can become very peculiar , compact stars , either white dwarf stars or neutron stars ; but if their final mass is too large , they collapse indefi- nitely , becoming ...
... becoming much smaller . If their final mass is small enough , they can become very peculiar , compact stars , either white dwarf stars or neutron stars ; but if their final mass is too large , they collapse indefi- nitely , becoming ...
Page 229
... become of the same order as the second wavelength . Thus , the problem becomes more one of kinetic theory than one ... become so widespread that results derived with it have become a ubiquitous part of the environmental impact studies re ...
... become of the same order as the second wavelength . Thus , the problem becomes more one of kinetic theory than one ... become so widespread that results derived with it have become a ubiquitous part of the environmental impact studies re ...
Page 301
... becoming proportional to ( z / L ) 3 . This means that σ increases with height , and the vertical angle σ / V , which ... become large again . This is believed to be a result of gravity waves rather than turbulence . As a result , dur ...
... becoming proportional to ( z / L ) 3 . This means that σ increases with height , and the vertical angle σ / V , which ... become large again . This is believed to be a result of gravity waves rather than turbulence . As a result , dur ...
Contents
Guide to Using the Encyclopedia ix Atomic Physics | 339 |
Approximations and Expansions 1 Atomic Spectrometry | 357 |
Archaeological Geology 31 Atomic Spectroscopy | 381 |
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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