The Hyades Kinematical Structure with Gaia Era
DOI:
https://doi.org/10.56042/ijpap.v60i3.58781Keywords:
Stars kinematics and dynamics, Stars distances, Galaxy structureAbstract
In this work, we have improved the Hyades members with crossmatch between Hipparcos and the recent Gaia EDR3 source, the obtained members with highly probable are about 186 candidates. Considering the classical convergent point and depending on proper motions and radial velocities, we have computed the apex position which is in line with others. The internal structural parameters of the Hyades open cluster are demonstrated here with space spatial velocities; i.e., (-5.97±0.41, 45.54±6.75, 5.52±0.43) and (-42.11±6.50, -19.09±4.37, -1.32±0.44) and on basis of matrix elements , the Velocity Ellipsoid Parameters were achieved, e.g., and . For the observational quantities, we have deduced a correlation coefficient of about for the kinematical property of proper motions on both sides and the physical property with the angular distances from the vertex, and those prove that the attributes are completely related linearly.
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