General Plastic Behavior and Approximate Solutions of Rotating Disk in Strain-hardening Range
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METALS - NICKEL ALLOYS↗
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Results for “Disks”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Signatures of planets: modeling structure in debris disks
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circumstellar disks SIRTF secular perturbation the↗
High angular resolution IR imaging of young stellar disks
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infrared stellar disks imaging↗
Debris disk imaging with NASA's SIRTF observatory
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circumstellar disks zodical dust SIRTF project↗
The photoionization of circumstellar disks
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circumstellar disks HII regions star formation↗
Resonant structure in the Kuiper Disk
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circumstellar disks Kuiper belt↗
Accretion shock in protostellar disk
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star formation protostar disk↗
VSOP Observations of a Sub-Parsec Accretion Disk
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VLBI VSOP Active Galaxies Interferometry Accretion↗
The effects of winds and photoionization on evolution of circumstellar disks
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star formation circumstellar disks HII regions out↗
Dust Evolution in Protostellar Accretion Disks
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hydrodynamics radiation transfer dust evolution ci↗
The Deuterium Chemistry in a Protoplanetary Disk
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circumstellar disks chemistry of deuterium↗
Modeling High Spatial Resolution Images of Protostellar Disks
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Star formation protostellar disks↗
A Sub-Parsec Accretion Disk in NGC 4261
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Sub-Parsec Accretion Disk Parsec Scale Nuclear Reg↗
A Sub-Pharsec Accretion Disk in NGC 4261
We observed the nuclear region of NGC 4261 (3C270) with the VLBA to determine the morphology of the central radio source on parsec scales.
Parsec Scale Accretion Disk Radio Source↗
Multi-Frequency VLBA Imaging of NGC4261's Accretion Disk
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central black hole↗
Evidence for Outflow-Infall Interactions Terminating Accretion in Protostellar Disks
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Outflow-Infall Accretion Protostellar Disks↗
A Model for Infall-Outflow Interactions in Protostellar Disks
Recently we have shown (sup 1,2) from (sup 12) CO and C (sup 18) O OVRO-MMA observations evidence of infall-outflow interactions in the Young Stellar Object IRS1 in B5. We present new data obtained with the OVRO-MMA in (sup 13) CO(2-1) and (1-0) to trace the full extent of this infall-outflow interaction region.
Protostellar Disks Young Stellar Object infall out↗
Detection of a Gap in the Circumstellar Disk, From High-Resolution Mid-Infrared Observations
The Herbig Ae star, AB Aur, was observed at 11.7(micro)m wavelength using the Cornell SpectroCam-10 imaging spectrometer on the 5-m Hale Telescope.
circumstellar disk infrared obervations mid-infrar↗