Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 123
... complex molecular chemistry and dust formation . It is plausible that they constitute one phase of dust in both stellar envelopes and winds , and in the interstellar medium . VI . Conclusions The field of observational astrochemistry is ...
... complex molecular chemistry and dust formation . It is plausible that they constitute one phase of dust in both stellar envelopes and winds , and in the interstellar medium . VI . Conclusions The field of observational astrochemistry is ...
Page 629
... complex numbers , which are numbers defined as having both real and imaginary parts . ( A more realistic complex num- ber class would have many more facilities , the simplifications imposed below are for clarity . ) class Complex ...
... complex numbers , which are numbers defined as having both real and imaginary parts . ( A more realistic complex num- ber class would have many more facilities , the simplifications imposed below are for clarity . ) class Complex ...
Page 712
... complex already containing the olefinic sub- strate as a coordinated ligand . geneous catalytic hydrogenation using catalysts , notably Rh ( I ) complexes , containing chiral phosphine ligands , such as Ph2PCH ( CH3 ) CH- ( CH3 ) PPh2 ...
... complex already containing the olefinic sub- strate as a coordinated ligand . geneous catalytic hydrogenation using catalysts , notably Rh ( I ) complexes , containing chiral phosphine ligands , such as Ph2PCH ( CH3 ) CH- ( CH3 ) PPh2 ...
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