Encyclopedia of Physical Science and Technology, Volume 2Robert Allen Meyers |
From inside the book
Results 1-3 of 18
Page 71
... molecular clouds , and ultimately new stars , will form . Be- cause the stars that are ejecting material are at the endpoints of their lifetimes , their envelopes are enriched in the heavy elements that were produced in their interiors ...
... molecular clouds , and ultimately new stars , will form . Be- cause the stars that are ejecting material are at the endpoints of their lifetimes , their envelopes are enriched in the heavy elements that were produced in their interiors ...
Page 72
... molecular cloud core . Since the dust temperature is quite low at this time ... clouds with masses in the range from 0.1 to 100 solar masses . Again , the ... clouds by IRAS have been suggested as protostellar objects , but this ...
... molecular cloud core . Since the dust temperature is quite low at this time ... clouds with masses in the range from 0.1 to 100 solar masses . Again , the ... clouds by IRAS have been suggested as protostellar objects , but this ...
Page 75
... molecular clouds ( Fig . 11 ) . This silicate dust may have its origin in the mass - loss from late - type M - stars discussed in Section V , D above . Many stars em- bedded in molecular clouds also show a 3.1 - μm absorption feature ...
... molecular clouds ( Fig . 11 ) . This silicate dust may have its origin in the mass - loss from late - type M - stars discussed in Section V , D above . Many stars em- bedded in molecular clouds also show a 3.1 - μm absorption feature ...
Contents
Executive Advisory Board ii BASIC Programming Language | 353 |
Editorial Advisory Board V Thomas E Kurtz | 373 |
Batteries | 387 |
Copyright | |
18 other sections not shown
Other editions - View all
Common terms and phrases
absorption acid aldoses angular momentum asbestos atmosphere atomic spectroscopy atoms auroral axis BASIC battery black hole Boolean algebra boundary layer carbon fibers catalyst cell charge chemical chrysotile clouds collision concentration cross section crystallites density disaccharide dust electric electron elements emission emitted energy engine equation example expert system field flux frequency function galaxies heat hemiacetal hydrogen hydroxyl groups infrared interaction interstellar interstellar medium ionized ions kinetic light magnetic mass material measurements mechanical ment metal method molecular molecules momentum monosaccharides motion nucleophile observed oligosaccharides operation optical orbit oxidation oxygen particles phase photons plane plume potential problem radiation reaction reactor region result saccharides sample satellite signal solar solution spectral spectroscopy spectrum speed stars stellar structure surface techniques temperature thermal tion transfer turbulence ture typical velocity vertical voltage wave wavelength wind