... б б Monday 25 . б 8:30 - M. Zwaan - Extragalactic science with ALMAб I . ... б 8:30 - M.E. Palumbo - Complex organic molecules in irradiated interstellar ice ... б 8:30 - M. Massardi/R. Paladino - Using the ALMA Science Archive data I . ...
... 3.6-, 4.5-, 5.8- and 8.0-m images on UT 2004 October 27 using the Infrared Array ... now argue that the 3.6- to 5.8-m points are dominated by an old stellar population ... We now use the H through to the 8.0-m SED of MRC 2104-242 to derive the most ...
... 8M sun 4R sun 10 3 L sun , i.e. earlier than B3) than low-mass ZAMS stars. ... in explaining the formation of low-mass stars, is not able to explain how a star with mass higher than ~8M sun can be formed ...
... near-infrared spectra from 0.8 to 2.4 Л m as obtained through a high-throughput ... 0.8 Л m 5. ... a very low-mass, embedded, late-M spectral type object (M~8-12 Mjup, AV=9 mag, M8.5 ...
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Ссылки http://www.arcetri.astro.it/~lt/projects/pres_arch/iau211-poster.PDF -- 1049.5 Кб -- 11.09.2007 Похожие документы
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... wavelength at the entrance pupil (corresponding to 0.8µm halo at 0.16 - 0.08 arcsec ... ratios are 1.0 в 10-6 at 0.5 arcsec for D=8m and 2 в 10-7 at 0.1 arcsec for D=30 m ...