Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 38
... studies be- came more sophisticated , owing to the applica- tion of optical microscopic techniques of min- eral identification . By the turn of the century these provenance studies were considered im- portant enough by classical ...
... studies be- came more sophisticated , owing to the applica- tion of optical microscopic techniques of min- eral identification . By the turn of the century these provenance studies were considered im- portant enough by classical ...
Page 150
... studies of en- tire galaxies . Such studies are often unfeasible for our own Galaxy . Sensitive ground - based NIR and TIR measurements require small ( 1-30 arcseconds ) photometer beams ; the time re- quired to map the star formation ...
... studies of en- tire galaxies . Such studies are often unfeasible for our own Galaxy . Sensitive ground - based NIR and TIR measurements require small ( 1-30 arcseconds ) photometer beams ; the time re- quired to map the star formation ...
Page 151
... studies of gal- axies are dominated by the hot young stars with very small mass - to - light ratios , whereas infrared studies reveal the old , low - luminosity popula- tions that have high mass - to - light ratios . Obser- vations in ...
... studies of gal- axies are dominated by the hot young stars with very small mass - to - light ratios , whereas infrared studies reveal the old , low - luminosity popula- tions that have high mass - to - light ratios . Obser- vations in ...
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