... limitation), two observations by Horch et al. (2002) with the 3.5m WIYN telescope at Kitt Peak, and 12 observations with the 6 ... To obtain a consistent orbit, we had to adjust the quadrants of measurements from the 2.1 m and the 3.5m telescopes. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/balega_etal_aua_hipparcosbinaries2_2006.pdf -- 386.6 Кб -- 05.05.2009 Похожие документы
... 0.461.4 µm and 1.42.5 µm with R 800 and 700, resp ectively, were obtained at the 3 ... lines of [O I] at 63.2 µm, [O III] at 88.5 µm, and of [C II] at 157.8 µm in the ISO ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2009/2009arXiv0904.1822M.pdf -- 553.9 Кб -- 18.05.2009 Похожие документы
... 08 (characteristic age = 10 7 years, distance d ~ 260 pc) - a candidate for optical identification, R=25.53 m 0.25, S/N ~ 3.5 ... PSR J0814+7429 ( = 10 8 years, d ~ 310 pc) - the limit of optical brightness of the object in R band is R c 25.5m . ...
... пк) - кандидат на оптическое отождествление, R=25.53 m 0.25, S/N ~ 3.5, необходимы дальнейшие BVI-наблюдения для подтверждения ... PSR J0814+7429 ( = 10 8 лет, d ~ 310 пк) -- в R-полосе предел на оптическую яркость объекта R c 25.5m . ...
... Accuracy of such estimations ranges within 0. 1 and 0. 5, m where it is worse than 0. 2 for most of them. ... 107, V=11. 3, Dm=0. 16 m 1 0 2 ±0. 09), photon bias amplitudes Cp <Cp <Cp and HR233 (r=0."016, V=5.m4, Dm=1.m 08±0.m08). ...
... speckle interferometry data obtained by J. Woitas with the 3.5m telescope of Calar Alto and covering an orbital arc of more ... A parallax of 4.8 mas would provide a total mass of 5.5M , expected for a pair of A1 V components. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/205349_web.pdf -- 136.4 Кб -- 05.05.2009 Похожие документы
... 5 a n d 1.5mm a g f r o m n i g h t t o n i g h t . ... e d a l o n g i t u d i n a l m a g n e t i c f i e l d w h i c h s l o w l y c h a n g e d f r o m + 5 0 0 G t o -- 1 0 0 0 G ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1996/1996_p86.pdf -- 43.7 Кб -- 21.04.2010 Похожие документы