... 7.7 µm (full line) and 11.3 µm (dashed line) emission features as functions of the ... 7 µm (full line) and 11.3 µm (dashed line) emission features as functions of column ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2005/MidIRSocorroNov05.pdf -- 1996.8 Кб -- 25.11.2009 Похожие документы
... of the nearby starburst NGC 520 in four narrow filters (7.9, 9.7 , 11.6 and 12.5 µ m ... at 7.9, 9.7 and 11.6 µ m) and 27thJuly (12.5 µ m filter) in photometric conditions ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2003/nam2003-aod2003-poster.pdf -- 1338.9 Кб -- 25.11.2009 Похожие документы
... mM 0.01 0.10 Data source: exoplanets.org SemiOrbital semi-major axis //AU U -majora axis A 1.00 10.00 p 100.00 Kepler-11: A ... 2011 Sun Kepler-32 system Kepler-11M Kepler-80 ju p 10Meart Meart 0.01 0.1 1 semi-major axis / AU h h 10 Why is this ...
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Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/THands.pdf -- 1345.6 Кб -- 16.04.2014 Похожие документы
... z x, y x, y z x , y z x, y z x , y z Allowed movement 0.11 arcsecond Insensitive Unconstrained 1.2-2µm 100µm 0.11 arcsecond 0.76 arcsecond 1.2-2µm 100µm Insensitive Unconstrained Limiting Requirement Position of image n/a n/a Position of image Quality of ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.TechMeet4/transmissiveLayouts.pdf -- 308.7 Кб -- 21.05.2010 Похожие документы
... Milne et al. 1989, PASAu, 8, 187. MOST at 843 MHz (43"?49": S=45?11), and Parkes 64-m at 8.4 GHz (3': S=19.5?1.0), including polarization. ADS . ...