... They are breaked, probably, stronger due to more favourable conditions, that is due to more accelerated tempo of mass loss or their field configuration was nearer to the dipole one, or due their being in a "tail" of maxwellian distribution P and etc. ...
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p83-p96.pdf -- 113.2 Кб -- 24.02.2010 Похожие документы
... Larger values of Yout affect the SED only in the far-infrared, i.e. far beyond the IRAS 25 µm photometric band, which defines the long-wavelength tail in this study. ...
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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
... Larger values of Y out af fect the SED only in the farinfrared, i.e. far beyond the IRAS 25 m photometric band, which defines the longwavelength tail in this study. ...
... In the I , R,and V bands, the shapes are typical of flare stars (Parenago 1956): the "tails" of the histograms on the bright side demonstrate that energetic flares are rare events. ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2006/shakhovskoj_etal_aua_dftau_2006.pdf -- 535.7 Кб -- 24.02.2010 Похожие документы
... 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://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2007/aa6224-06.ps -- 1272.8 Кб -- 24.02.2010 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://jet.sao.ru/hq/balega/PUBL_BAL/PUB_1999/1999A&A_348_805B.pdf -- 387.4 Кб -- 24.02.2010 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://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_529H.pdf -- 322.5 Кб -- 24.02.2010 Похожие документы