Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 143
... mass - loss rate of matter from the star . Table III summa- rizes the results of this technique as applied to late - type stars , early - type stars , and novae . Be- cause most of the stars in this table have masses between 1 and 10 ...
... mass - loss rate of matter from the star . Table III summa- rizes the results of this technique as applied to late - type stars , early - type stars , and novae . Be- cause most of the stars in this table have masses between 1 and 10 ...
Page 515
... Mass Transfer and Mass Loss in Binaries VI . X - Ray Sources and Cataclysmics VII . Formation of Binary Systems VIII . Concluding Remarks GLOSSARY Accretion disk : Structure formed when the material accreting onto a star has excess ...
... Mass Transfer and Mass Loss in Binaries VI . X - Ray Sources and Cataclysmics VII . Formation of Binary Systems VIII . Concluding Remarks GLOSSARY Accretion disk : Structure formed when the material accreting onto a star has excess ...
Page 564
... mass of the compact object at 10 solar masses . It is an excellent candidate for a black hole . IV . Black Hole Evaporation In the 1970s it was noted that the classical laws governing the interaction of a black hole with its ...
... mass of the compact object at 10 solar masses . It is an excellent candidate for a black hole . IV . Black Hole Evaporation In the 1970s it was noted that the classical laws governing the interaction of a black hole with its ...
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