... HIP 96656 [# = 19 h 39 m 06.4 s , # = +76 # 25 # 19 ## (2000), K1V, m V = 8.08] has attracted attention over the past two decades as an additional good candidate for a comparison with de tailed evolutionary calculations in the discussed mass range ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2007/aa6224-06.ps -- 1272.8 Кб -- 06.05.2009 Похожие документы
... This is due to the fact that larger particles increase the curvature of the visibility curve at low spatial frequencies whereas the highfrequency tail (the plateau) is found at lower visibility values. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_1999/1999A&A_348_805B.pdf -- 387.4 Кб -- 05.08.2004 Похожие документы
... However, the spectral index of the far-infrared tail of the SED and the visibilities seem to favour the above flat density distribution in the outer shell region rather than a superwind component. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_529H.pdf -- 322.5 Кб -- 03.08.2004 Похожие документы
... The choice of the grain radius only affects the short wavelength tail of the SED below < 3 µm, because at these wave lengths ext /Vgr still depends on agr , but it becomes independent of agr at longer wavelengths (see Fig. ...
... High-resolution spectra of the atmospheres had been smoothed out to / 100 and extrapolated using their slopes at 12 µm to longer wavelengths until they intersect the Rayleigh-Jeans tail of a blackbody of the same temperature and luminosity. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_368_497M.pdf -- 1354.2 Кб -- 03.08.2004 Похожие документы