... noting that the primary mirror of the LBT is located 35m above the dome of the VATT ... m. In conclusion, the main HVRGS concept consists of (i) taking a wide binary of the ...
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Ссылки http://www.arcetri.astro.it/~masciadr/PUBLI/masciadri2010.pdf -- 1052.6 Кб -- 16.08.2010 Похожие документы
... 7 cm 3.6 cm 6 cm 0.7 cm 3.6 cm 6 cm UX Ori CQ Tau Phase center ff(J2000) 05 h 04 m 29.99 s 05 h 35m 58.47 s ffi(J2000) \Gamma03 ffi 47 0 14.3 00 +24 ffi 44 0 54.1 00 Observing date 10Sep00 05Sep00 10Sep00 02Oct00 02Oct00 05Oct00 Configuration D D D D D D ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/uxors_vla/uxors_vla.ps.gz -- 167.2 Кб -- 11.09.2007 Похожие документы
... Although excitation by 35-m infrared (IR) photons can also populate the 3s2 3p 2 P3/2 excited level, it seems unlikely that ... for populating the 3s2 3p 2 P3/2 Si II level, then a specific luminosity at 35m of 1039 erg s-1 Hz-1 would be required ...
... 15 3.M.RC MAGGIO 2015 MA LP/PPB 5 I.N.A.F. ISTUTUTO NAZIONALE DI ASTROFISICA RISTRUTTURAZIONE OFFICINA MECCANICA IMPIANTI MECCANICI RELAZIONE DI CALCOLO - Illuminazione spogliatoi ONAMENTO GIORNALIERO DEGLI IMPIANTI 35 W / m q. FUNZI - Sezione meccanica ...
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Ссылки http://www.arcetri.astro.it/~migliett/Appalti/LAB_OA_DOCS/3.M.RC.pdf -- 797.9 Кб -- 28.05.2015 Похожие документы
... mass ratio of log10 (Md /M ) = -3.35, indicating lower dust fractions on average in ... this relation to purely star-forming galaxies as log(sSF R ) = -0.35 log M - 6.33 ...
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Ссылки http://www.arcetri.astro.it/~sperello/2015MNRAS451_3815.pdf -- 2633.2 Кб -- 20.07.2015 Похожие документы