... This design concept of the phase plate positioning, realized in the SCORPIO-2, in contrast to the FORS spectrograph of the 8-m VLT telescope ([3, 4]) and the FOCAS spectrograph of the 10-m SUBARU telescope ([5]) is advantageous in that it does not ...
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Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio-2/manuals/AstrBull_2012_67_438.pdf -- 998.4 Кб -- 07.10.2013 Похожие документы
... 12.3 20 20.8 59.6 log L [L ] 5.61 5.68 5.76 5.7 5.89 5.8 log Mcl [M yr-1 ] -4.5 -4.8 -4.58 -4.75 -4.4 -4.63 f 0. 0. 0. 0. 1 1 1 ... For the two states, M differ by a factor 2.8, and the wind velocity is 1.8 times larger for the hot state. ...
... It will suce to mention the EFOSC camera of the 3.6-m ESO telescope (Buzzoni et al. 1984); in many respects, it became the prototype of modern spectrographs for 8-10-m telescopes, such as FORS on VLT (Nicklas et al. ...
... stronger than 5 m/s. The upper limit for the pulsations in the vicinity of the photometric frequency of HD 103498 is only 2.8m/s. In most of roAp stars the lines of the REE in the first and second ionization stages usually show the highest RV amplitudes ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p330.pdf -- 1235.2 Кб -- 11.08.2011 Похожие документы
... 2 5 7 , 8 0 A n g e l J . R . P . : 1 9 7 8 , " M a g n e t i c w h i t e d w a r f s " I n : A n n u . R e v . A s t r o n . A s t r o p h y s . ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1996/1996_p11.pdf -- 188.6 Кб -- 21.04.2010 Похожие документы
... scanning IFP were employed in observations at many big telescopes (TAURUS2 at the 4.2 m telescope WHT (Spain), PUMA at the 2.1 m telescope of OAN (Mexico), CIGALE at the 3.6m telescope (ESO), the pro ject KTS for the Japanese 8.2 m telescope SUBARY, etc ...
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Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio-2/manuals/0211104.pdf -- 900.1 Кб -- 16.08.2013 Похожие документы