Zobrazeno 1 - 10
of 14
pro vyhledávání: '"G. H. Stokes"'
Publikováno v:
Space 2000.
Publikováno v:
Space 98.
Lincoln Laboratory has a long history of developing electro-optical space surveillance technology for resident space object search, detection, orbit determination, and catalog maintenance. Recent advances in large format, highly sensitive CCDs make p
Publikováno v:
Engineering, Construction, and Operations in Space V.
Autor:
G. H. Stokes, D. F. Kostishack
Publikováno v:
Annals of the New York Academy of Sciences. 822:544-544
Autor:
R. J. V. Brissenden, James Taylor, N. D’Amico, J. M. Durdin, D. R. Stinebring, Richard N. Manchester, G. H. Stokes
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 234:437-443
L'exploration d'une zone le long du plan galactique sud (P=255° a P=360°, b=±1°) a ete effectuee par le radiotelescope de Molonglo pour la recherche de pulsars millisecondes. Un total de 10 pulsars ont ete detectes dont un nouveau pulsar, PSR 090
Publikováno v:
Nature. 322:712-714
Much of the interesting physics concerning neutron stars and their evolution depends for its experimental foundation on observations of the rotation rates of pulsars. To continue recent efforts of our group in this area1–3, we began a series of pul
Publikováno v:
American journal of veterinary research. 37(6)
Crude hemolysin derived from Listeria monocytogenes, strains 9-125 and 1122-3, reduced phosphate utilization of rat brain mitochondria in a succinate system. Oxidation rates were not altered by addition of hemolysin to a concentration of 42 hemolytic
Autor:
G H, STOKES
Publikováno v:
The Jefferson-Hillman hospital bulletin. 2(4)
Publikováno v:
Nature. 317:787-788
All extensive pulsar surveys to date1–5 have had sensitivities that deteriorate rapidly for periods P shorter than a few-tenths of a second, and none of them has had any appreciable sensitivity for P
Publikováno v:
The Astrophysical Journal. 311:694
Results are reported from two surveys designed to detect fast pulsars - one carried out at 390 MHz using the 92 m telescope at Green Bank, and the other done at 430 MHz with the 305 m Arecibo antenna. Twenty-five new pulsars were discovered. Six puls