Science: v.1-v.219Moses King, 1970 |
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Стр. 1205
... galaxies , broken only in rare places by an occasional large globular cluster of galaxies , a few megaparsecs across , of which the nearest and best known ex- ample is in Coma . These great clusters , being easy to recognize at large ...
... galaxies , broken only in rare places by an occasional large globular cluster of galaxies , a few megaparsecs across , of which the nearest and best known ex- ample is in Coma . These great clusters , being easy to recognize at large ...
Стр. 1208
... galaxy counts are available . Nu- merical details and. system of observed radius R may be called the Schwarzschild filling factor . For most common astronomical bodies ( stars ) or systems ( galaxies ) , the filling factor is very small ...
... galaxy counts are available . Nu- merical details and. system of observed radius R may be called the Schwarzschild filling factor . For most common astronomical bodies ( stars ) or systems ( galaxies ) , the filling factor is very small ...
Стр. 1209
... galaxies ( 39 ) . If we consider all clusters with a characteristic radius RdR , there is apparently an upper limit to the space density of galaxies VR or to the mass density PR that can exist within the corresponding volume ; this ...
... galaxies ( 39 ) . If we consider all clusters with a characteristic radius RdR , there is apparently an upper limit to the space density of galaxies VR or to the mass density PR that can exist within the corresponding volume ; this ...
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