Science, Volume 291John Michels (Journalist) American Association for the Advancement of Science, 2001 |
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Page 82
... lines from the presumed host galaxy . The energy is derived from the y - ray fluences reported and assumes that the GRB emitted energy isotropically . [ Courtesy of J. S. Bloom and the Caltech GRB group ] 801 - Amplification 802 ...
... lines from the presumed host galaxy . The energy is derived from the y - ray fluences reported and assumes that the GRB emitted energy isotropically . [ Courtesy of J. S. Bloom and the Caltech GRB group ] 801 - Amplification 802 ...
Page 496
... lines , yel- low expression was higher than that in the control ESY lines , and in three lines it was at wild - type levels . When three of the less pig- mented ESFSY were tested in a su ( Hw ) background , wild - type pigmentation was ...
... lines , yel- low expression was higher than that in the control ESY lines , and in three lines it was at wild - type levels . When three of the less pig- mented ESFSY were tested in a su ( Hw ) background , wild - type pigmentation was ...
Page 625
... lines of ions , which imply fairly high excitation temperatures . We suggest that an ion formation mechanism , based on reso- nance - enhanced two - photon ionization ( RETPI ) by intense H Lyman a radiation ( wavelength of 1215 ...
... lines of ions , which imply fairly high excitation temperatures . We suggest that an ion formation mechanism , based on reso- nance - enhanced two - photon ionization ( RETPI ) by intense H Lyman a radiation ( wavelength of 1215 ...
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