... Below the threshold, collisions take over and deflect e+ in their motion parallel to magnetic-field lines. ... On average, there is neither gain nor loss in energy and e+ diffuse over a distance = 2D along magnetic-field lines until they annihilate directly with bound e- ( is the e+ lifetime [7]). ... Average distance z travelled by e+ during the slowing-down period and spatial dispersion of the distribution z 2 1/2 in the warm ionized and hot ionized phases. n is the total gas density. ...

Distant globular clusters with anomalously small masses. ... We found that 10 metal-poor globular clusters are greately distinguished for anomalously small masses on the "destruction rate-mass" plain. ... Note that 10 distant clusters of anomalously small mass selected by us proved to be younger and with an average metallicity <[Fe/H]> = -1.36 ? ... It looks as if only far from the centre of the Galaxy, conditions are created that lead to formation of globular clusters with anomalously small masses. ...

... Printed below is the GNU General Public License (the GPL or copyleft), under which Linux is licensed. ... GNU GENERAL PUBLIC LICENSE . ... This General Public License applies to most of the Free Software Foundation's software and to any other program whose authors commit to using it. ... This License applies to any program or other work which contains a notice placed by the copyright holder saying it may be distributed under the terms of this General Public License. ...

... Reports on progress and error are always recorded in the log file of the program. ... UT date of the measurement finish in YYYY-MM-DD format UT time of the measurement finish in hh:mm:ss format Average flux in A aperture Average flux in B aperture Average flux in C aperture Average flux in D aperture Normalized variance of flux in A aperture Normalized variance of flux in B aperture Normalized variance of flux in C aperture Normalized variance of flux in D ...

Annu. ... Key Words stellar energy production, Nobel Prize, supernova, binary pairs s Abstract Astrophysics has been an important part of my personal and scientific life three times. ... Gamov suggested to one of his graduate students, Charles Critchfield, that he actually calculate the proton-proton reaction. ... In stars, the proton-proton reaction is usually followed by a chain of reactions with the end result of producing 4He. ... In 1938, they suggested energy production in stars. ...