... 3 20 s 25 s 30 s 35 s 40 s 45 s 5 37 50 h m s +35 37' o 38' 39' 40' 41' 42' 43' Fig ... the errors quoted 30 s 31 s 32 s 5 37 33 h m s +35 40'00" o 20" 40" +35 41'00" o 20 ...
... 48.9 ± 7.6 m was only 14 m higher than the observed one (hsl,obs = 35.3 ± 5.1 m ... computed in grid-nested mode is closer to the observed one (hsl,obs = 35.3 ± 5.1 m ...
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Ссылки http://www.arcetri.astro.it/~masciadr/PUBLI/lascaux_et_al2010.pdf -- 771.2 Кб -- 27.01.2012 Похожие документы
... rather good values for the seeing above 30-35m: around 0.3 arcsec at Dome C. Site ... to the observed one (hsl,obs = 35.3 Б 5.1 m), while the grid-nested technique is ...
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Ссылки http://www.arcetri.astro.it/~masciadr/PUBLI/lascaux2009.pdf -- 1759.4 Кб -- 17.12.2009 Похожие документы
... Ad ogni settima striscia della griglia si ha un'azione piu' intensa pari a un multiplo della prima come un cosiddetto secondo ordine: quindi alla distanza di 28 ovvero 35m e 35 ovvero 42 m." . ...
... 6.6 6.6 35 11 390 56 1.3 28 31 37 Units 1013 cm~2 1022 cm~2 M _ km s~1 M km s~1 ... Containing 35M of material, this compact outяow is over an _ order of magnitude ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/afgl5142_2/afgl5142ovro.pdf.gz -- 431.4 Кб -- 11.09.2007 Похожие документы
... suggest that these masers are tracing rotation around a central mass of about 35M ... Assuming centrifugal equilibrium the required central mass is 35M . ... The inferred dynamical mass (35M ) is consistent with 6.7 GHz masers tracing a high ...
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Ссылки http://www.arcetri.astro.it/science/starform/preprints/mosca_03.pdf -- 695.2 Кб -- 10.05.2010 Похожие документы
... Baselines between 35m and 11.4 km could detect a largest angular emission scale, LAS 18 00 . ... Baselines between 35m and 3.4 km provided a synthesized beam of approximately 0:4 00 over the 1 0 eld of view. ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/w75n_sio/w75n_sio.ps.gz -- 503.4 Кб -- 11.09.2007 Похожие документы