... 2SB 2SB 2SB 2SB 2SB DSB DSB 3 Supplier HIA NAOJ OSO NRAO IRAM NAOJ NOVA NAOJ 4 1 3.1 Computing the dispersive path delay We ... USA; IRAM - Institut de Radio Astronomie MillimИtrique, France; NOVA Nederlandse Onderzoekschool voor de Astronomie ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2009/ALMAMemo590.pdf -- 908.6 Кб -- 10.08.2012 Похожие документы
... D., Davis R. J., Feroz F., G nova-Santos R., Grainge K. J. B., Green D. A., Hobson M ... D., Davis R. J., Dickinson C., G nova-Santos R., Grainge K., Hafez Y. A., Hobson M ...
... A. Quirrenbach, N. M. Elias, D. Mozurkewich, J. T. Armstrong, D. F. Buscher, and C. A. Hummel, Observations of nova cygni 1992 with a long-baseline interferometer, Astron. ...
... Occasional explosions, thought to be due to thermonuclear runaways on the white dwarf, characterise the nova activity. ... Around three nova outbursts are expected to be observable each year, offering many opportunities for detailed study. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf -- 1989.2 Кб -- 25.06.2007 Похожие документы