... At a wavelength of = 2.13 µm the diffraction-limited resolution of 74 mas was ... stellar contribution to the total flux at = 2.13 µm is less than 30% at all phases ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf -- 428.8 Кб -- 24.02.2010 Похожие документы
... following absolute magnitudes for the components: M IA =10.5, M IB =12.9, M IC =14.2 ... star for the first time using the speckle interferometer at the 6 m BTA telescope [2 ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2006/malogolovets.ps -- 808.5 Кб -- 24.02.2010 Похожие документы
... 4.0 M log L/Lo 2.5 2 3.0 M o Bs 2.5 M o o 4900 4800 1.5 4700 2.0 Mo 4600 1.5 Mo 4.2 ... 11000 10500 log L/Lo 10000 3.0 M o 2 Bs 9500 2.5 M o 1.5 9000 1 2.0 Mo 8500 1.5 Mo ...
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/2003/2003_p121.pdf -- 394.2 Кб -- 21.04.2010 Похожие документы
... COMPLEX OF 2-m TELESCOPE SPECTRAL EQUIPMENT FOR RESEARCH OF THE INTERSTELLAR ENVIRONMENT OF PEAK TERSKOL OBSERVATORY MUSAEV F.A ... MAESTRO echelle spectrometer was mounted in the coude focus (F/36) of the 2-m telescope in 1997. ...
... 3 4 5 6 10-1 10-1 10-1 10-1 C 0 1 2 3 10 10 n, cm 10 3 10 103 104 n, cm 105 3 106 1 = m -0 -200 2 104 -400 -800 m u = - 2 - 2m b 1 .4 = m ff u= c nH, cm3 b2 + 2 c 2 b 22 b m v, cm/s -600 -1000 -1200 -1400 -1600 10 17 103 f(H)=0.1 f(H)=0.2 f(H)=1.0 r ...
... the first diffractionlimited 2.13 m speckle interferometric observations of WR 118 ... 0.525 m, and our 2.13 m visibility function, assuming spherical symmetry of the ...
... the first diffraction-limited 2.13 µm speckle interferometric observations of WR 118 ... 0.525 µm, and our 2.13 µm visibility function, assuming spherical symmetry of the ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_229Y.pdf -- 168.2 Кб -- 24.02.2010 Похожие документы