... for the flux between 2 and 10 µm and for > 20 µm. A good fit was found for Y = 6.5 ... Second, the flux beyond 20 µm is somewhat too low. ... 9.2 log (*F) [Wm-2] 0 1 [µm] 10 100 -9.3 -9.4 -9.5 -9.6 -9.7 -9.8 10 [µm] 20 30 Fig ...
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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
... Single-shell models -9.8 2 3 4 5 10 [µm] 20 30 40 50 Fig. 5. ... incomplete due to a lack of sufficiently high fluxes at longer wavelengths ( > 20 µm ... close enough to raise the fluxes at > 20 µm but distant enough in order to preserve ...
... turned out to underestimate the flux beyond 20 µm. A two-component model existing of ... the size of CIT 3 at 2.2 µm, 10 µm, and 20 µm by means of lunar occultations ...
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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
... for the wavelength region from 1 µm to 20 µm is available in the literature for AFGL ... range from = 1.2 µm to = 20 µm is only fully covered by observations around phase 0 ...
... the optical brightness contrast between a Mw 5 20M( primary star and a Mw 5 1 M ... simulations with primary masses of 10 M( and 20M( and found no significant changes ...
... Beichman et al. (1979) resolved the 20 µm infrared emission into three individual ... near-infrared emission, were not detected at 20 µm. Therefore, Evans et al. (1989 ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_381_905W.pdf -- 418.9 Кб -- 24.02.2010 Похожие документы
... Beichman et al. (1979) carried out 20 µm observations of this region and were able to resolve the infrared emission into three ... At 20 µm, the dominant source IRS1 is 710 times brighter than the two other sources IRS2 and IRS3. ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2000A&A_361L_29S.pdf -- 286.3 Кб -- 24.02.2010 Похожие документы