... of the extragalactic sources seen through the Galacticplane (|b| 10 ) at 2, 5 and 8 ... to investigate the scattering properties within and outside the Galacticplane ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/mnras2015_452,4274.pdf -- 954.6 Кб -- 24.02.2016 Похожие документы
... The second corresponds to a cavity of depleted electron density extending as far as 300 pc from the Sun in the direction perpendicular to the galacticplane and 50100 pc in the Galacticplane 1 (component B; Snowden et al. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/apj2014_786_2_115.pdf -- 690.1 Кб -- 06.05.2014 Похожие документы
... From orbits consistent with this limitation and with the date of the launch October 1, 2000 as an example, an orbit was selected with apogee directed to the North Galactic pole at the begining and rotation of orbit plane was maximized. ...
... 2002); we take as typical values scatt 30 as at = 6 cm , scatt 300 as at = 18 cm , and scatt 8000 as at = 92 cm , which are approximately the median of the NE2001 angular broadening and, thus, represent typical lines of sight away from the Galacticplane ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/apj2015_805_2_180.pdf -- 1270.6 Кб -- 30.06.2015 Похожие документы
... The small difference between measured Tsys when observing calibrators and other objects can be referred to the cor responding background excess near the Galacticplane because the most studied sources are extragalactic. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2014,52,393.pdf -- 383.0 Кб -- 07.10.2014 Похожие документы
... Among OH masers at 1665 MHz unresolved galactic objects are W48 (25 Jy, 2 kHz) and G ... provided the largest rotation of the orbital plane around the axis of apsides, and a ...
... impulse-response function due to scattering, when sampled at the observer plane [1 ... has a characteristic scale in the observer plane LI SS that reflects the relative ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/tmp/evn%202014_064.pdf -- 207.5 Кб -- 17.06.2015 Похожие документы