Nature, Volume 434 |
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Page 192
note that the Arches stars are relatively unevolved ; indeed , only the An upper limit to the masses of stars ... STScI , 3700 San Martin Drive , Baltimore , Maryland 21218 , US There is no accepted upper mass limit for stars .
note that the Arches stars are relatively unevolved ; indeed , only the An upper limit to the masses of stars ... STScI , 3700 San Martin Drive , Baltimore , Maryland 21218 , US There is no accepted upper mass limit for stars .
Page 193
The frequency distribution generally decreases with increasing mass , and is fitted by two lines through the four most ... For both slopes , there appears to be a deficit of expected very massive stars with masses beyond ~ 130 Mo ...
The frequency distribution generally decreases with increasing mass , and is fitted by two lines through the four most ... For both slopes , there appears to be a deficit of expected very massive stars with masses beyond ~ 130 Mo ...
Page 827
Critical mass : Carol Robinson pushes the limits of a mass spectrometer to characterize large protein complexes . ... Carol Robinson F rom an early age I have been fascinated by the workings of a mass spectrometer .
Critical mass : Carol Robinson pushes the limits of a mass spectrometer to characterize large protein complexes . ... Carol Robinson F rom an early age I have been fascinated by the workings of a mass spectrometer .
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Contents
eating at heart p | 37 |
letters to nature | 50 |
Mesozoic Alpine facies deposition as a result | 59 |
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