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Boosting the velocity detection limit of 3D single-cell tracking time-lapse MRI by balanced SSFP imaging. [PDF]
Magn Reson MedWilken E +5 more
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A systematic approach for quantitative orientation and phase fraction analysis of thin films through grazing-incidence X-ray diffraction. [PDF]
J Appl CrystallogrGasser F +8 more
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Learning based prediction of cuttings concentration for enhancing hole cleaning efficiency in eccentric and deviated wells. [PDF]
Sci RepSaad MY +3 more
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Precision analysis of NGC 2158 with Gaia DR3. [PDF]
Sci RepAhmed NM, Tadross AL.
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Electrical double layer induced zeta potential effect in a disk cone system with surface catalyzed reaction. [PDF]
Sci RepRiasat S +6 more
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Revisiting the inverse Abel integral for reconstructing velocity-map images.
Phys Chem Chem PhysSparling C, Onvlee J.
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, 2015 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
D. Latham, N. Haghighipour
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Radial Velocity Measurements with FXCOR
Astrophysics and Space Science, 1998We present measured radial velocities of two peculiar early B type stars, to check their membership to the open cluster NGC 663. The radial velocities have been obtained with the cross correlation technique, using as a template stars from the list of Liu et al. (1989).
Rodes Roca, José Joaquín +2 more
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