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CFD-Based Evaluation of Stirred Tank Designs for High-Viscosity Copolymer Aramid Dope Mixing. [PDF]
Polymers (Basel)Yeo DH, Yoon HS, Yu SH, Sim JH.
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V3101 Cyg: A Cataclysmic Variable Born with a Brown Dwarf Donor
Ramirez S +7 more
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2014
In a system consisting of a star and a planet, because of the gravitational force of the planet on the star, the planet and its host star orbit their common center of mass. This causes variations in the distance of the star to the observer creating what is known as radial velocity. Measuring the velocities of stars along the line of sight dates back to
David W. Latham, Nader Haghighipour
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In a system consisting of a star and a planet, because of the gravitational force of the planet on the star, the planet and its host star orbit their common center of mass. This causes variations in the distance of the star to the observer creating what is known as radial velocity. Measuring the velocities of stars along the line of sight dates back to
David W. Latham, Nader Haghighipour
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30. Radial Velocities (Vitesses Radiales)
Transactions of the International Astronomical Union, 1988The present report on the activities of IAU Commission 30, covering the triennium June l, 1984 through June 1, 1987, will be somewhat different from its recent predecessors in both content and style. Over the preceding decade or so, the reports mainly emphasized the dramatic improvements in observing efficiency, achieved primarily through the general ...
J. Andersen +6 more
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International Astronomical Union Colloquium, 1984
AbstractThe writer reviews the presently available lists of standard-velocity stars approved by IAU Commission 30 and suggests that the time has arrived for major revisions. Many of the currently adopted standards are known or suspected to be variable in velocity at the level of precision to which we can now work. The writer suggests that we need three
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AbstractThe writer reviews the presently available lists of standard-velocity stars approved by IAU Commission 30 and suggests that the time has arrived for major revisions. Many of the currently adopted standards are known or suspected to be variable in velocity at the level of precision to which we can now work. The writer suggests that we need three
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Publications of the Astronomical Society of the Pacific, 1983
A number of techniques for determining stellar radial velocities with a precision better than 100 m s-1 are now becoming available. Three types of precision velocity techniques have been proposed, using for wavelength reference either telluric lines, Fabry-Perot fringes, or lines generated in an absorption cell. The author has used the latter technique,
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A number of techniques for determining stellar radial velocities with a precision better than 100 m s-1 are now becoming available. Three types of precision velocity techniques have been proposed, using for wavelength reference either telluric lines, Fabry-Perot fringes, or lines generated in an absorption cell. The author has used the latter technique,
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RVS' RADIAL VELOCITIES ACCURACY
EAS Publications Series, 2002D. Katz, Y. Viala, A. Gomez, D. Morin
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