Determination of Regge trajectories in a bootstrap model of pion-pion scattering

1967 ◽  
Vol 205 (2) ◽  
pp. 145-148
Author(s):  
Harald J. W. M�ller

1972 ◽  
Vol 5 (5) ◽  
pp. 1235-1235 ◽  
Author(s):  
C. J. Hamer ◽  
S. C. Frautschi


1971 ◽  
Vol 4 (7) ◽  
pp. 2125-2137 ◽  
Author(s):  
C. J. Hamer ◽  
S. C. Frautschi


1968 ◽  
Vol 58 (3) ◽  
pp. 639-643 ◽  
Author(s):  
S. Focardi ◽  
G. Mandrioli


1969 ◽  
Vol 12 (3) ◽  
pp. 567-572 ◽  
Author(s):  
P. Castoldi
Keyword(s):  




1966 ◽  
Vol 87 (5) ◽  
pp. 433-443 ◽  
Author(s):  
J. Pišút ◽  
P. Lichard ◽  
P. Bóna


Development ◽  
1983 ◽  
Vol 76 (1) ◽  
pp. 139-146
Author(s):  
Hans Meinhardt

For the sequential determination of proximodistal structures during the outgrowth of vertebrate limbs, a ‘bootstrap’-mechanism is proposed: by increasing feedback of more distally determined cells onto the production of a morphogen at the apical ectodermal ridge a successive increase of the morphogen concentration is achieved during outgrowth. The model accounts for the formation of a progress-zone at the limb tip, for the correct regeneration after truncation, for the presence and absence of proximodistal intercalation after certain graft experiments in amphibian limbs, for the tendency with which distal structures form in proximal position after certain experimental manipulations and for the intimate coupling of the anteroposterior and the proximodistal axes.



1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.



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