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CN and CH Band Strength Variations in M71 Giants

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CN and CH variations among red giants in the globular cluster NGC 6171

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CNES R&D Activities in support of Image Information Mining

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CNES-DLR Activities in Information Extraction for High-Resolution Image Understanding

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CNO abundances and hydrodynamic models of the nova outburst. II - 1.00 solar mass models with enhanced carbon and oxygen

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CO line emission from shock waves in molecular clouds

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CO line formation in bipolar flows. II - Decelerated outflow case and summary of results

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CO line formation in bipolar flows. III - The energetics of molecular flows and ionized winds

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Co-adding techniques for image-based wavefront sensing for segmented-mirror telescopes

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Co-clustering for Directed Graphs; the Stochastic Co-Blockmodel and a Spectral Algorithm

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Co-linear deuterium propulsion: An attainable variant to the Bussard Ramscoop

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Co-occurrence Matrix and Fractal Dimension for Image Segmentation

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Co-phasing and co-aligning the Multiple Mirror Telescope.

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Co/Ni Ratio in Galactic Cosmic Rays: Results from the TIGER-2001 Flight

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CO2 Chemistry in the Atmosphere of HD189733b

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CO2 gas fluidization in the initiation and formation of Martian polar gullies

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Coalescence Of 2, 3, Or More, Of Approx. 15 Heat Sources (Sustained By Radioactive Decay) Migrating Over Earth's Solid Inner Core Boundary, When Located Near Rotation Axis, In N- Or S-Hemisphere, Engenders Geomagnetic Field Reversals.

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Coalescence of Black Hole-Neutron Star Binaries

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Coalescence of self-gravitating gaseous masses - A numerical model

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Coalescing binary neutron stars

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