... MEM iterations S .. ... empty]test.mol Rest wavelength:[0= 6562.76] 6562.76 MOLLY File opened : test.mol Error reading MOLLY headers 43 spectra read. ... If unknown, use your best guess for (radial velocity ); you can check this using different values in modmap . (250 pixels at 0.8angstroms/pixel; better to oversample) modmap v Rest wavelength (A) : 6562.75788 Gamma velocity : -44 Number of pixels in velocity grid : 100 Maximum velocity in tomogram: 2000 FWHM of local line profile: 100 ...
ФИЗИЧЕСКИЕ ДАННЫЕ . СПУТНИКОВ УРАНА . ... 13.70 + 0.04 . ... The masses of Uranus and its Major Satellites from Voyager Tracking Data and Earth-based Uranian Satellite Data," Astronomical Journal 103 , 2068. ... Voyager's Eleventh Discovery of a Satellite of Uranus and Phometry and the First Size Measurements of Nine Satellites", Icarus 151 , 69-77 . ... Uranus Satellites: Surface Properties", In Uranus (J. T. Bergstralh, E. D. Miner, and M. S. Matthews Eds.) pp. ...
Magnetic stars, 2004, 198-204 Spectrophotometry of the He-weak star HD 217833 Glagolevskij Yu. ... From measurements made by Glagolevskij , Chunakova (1985) the star has a strong magnetic field varying from -2000 to -5000 G. Glagolevskij (2002) and Glagolevskij , c Sp ecial Astrophysical Observatory of the Russian AS, 2004 SPECTROPHOTOMETRY OF THE HE-WEAK STAR HD 217833 199 Table 1: Parameters of the He-weak star HD ... This is why it can be ranked among extreme He-weak stars. ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/2003/2003_p198.pdf -- 141.6 Кб -- 21.04.2010
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Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/2003/2003_p198.pdf -- 141.6 Кб -- 21.04.2010
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/2003/2003_p198.pdf -- 141.6 Кб -- 21.04.2010 Похожие документы
... Understand the shape and implications of the multiband ligth curve of GRB 050408, an Xray rich (XRR) burst. ... Together with Xray, millimetre and radio observations we compile what, to our knowledge, is the most complete multiband coverage of an XRR burst afterglow to date. ... The optical and Xray light curve is characterised by an early flattening and an intense bump peaking around 6 days after the burst onset. ... 2006; Chincarini et al. ... Optical observations carried out for GRB 050408. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2007/A&A_462_L57.ps -- 942.0 Кб -- 05.05.2009 Похожие документы
R And SiO maser. S And SN (NGC 224). W And SiO maser. Z And Outbursts, average cycle 8400d. Porb = 758.8d, it reveals Z And itself in photometry during the low state. A quasi-period, P1, Z And about 656d is present during the outbursts. The beat period Z And between Porb and P1, about 5500d, is also found in the Z And photometric data. RS And H2O maser. RT And Min II = 9.28. P varies, current elements are given. RU And P varies strongly. RX And Porb = 0.209893d. RY And OH, H2O maser. SS And P2 = 650d, P3 =