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The Hyades Kinematical Structure with Gaia Era

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Title The Hyades Kinematical Structure with Gaia Era
 
Creator Al-Johani, Amnah S.
Elsanhoury, W. H.
Al-Anzi, Aneefah
Al-Jaber, Bashayr
Al-Bishi, Fatmah
Kanaan, Nourah
Al-Atwi, Ragwa
Al-Khubrani, Reem
Al-Anzi, Sarah
 
Subject Stars kinematics and dynamics
Stars distances
Galaxy structure
 
Description 268-273
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 􀵫A􀭡􀭮, D􀭡􀭮􀵯 􀵌 􁈺93􀭭. 36 􀵇 0􀭭. 046, 7􀭭. 43 􀵇 0􀭭. 713􁈻
which is in line with others. The internal structural parameters of the Hyades open cluster are demonstrated here with space spatial
velocities; i.e., 􁈺 􀭜, V􀴥􀭝, V􀴥􀭞; km s􀬿􀬵􁈻 􀵌(-5.97±0.41, 45.54±6.75, 5.52±0.43) and 􁈺 , V􀴥, W􀴥 ; km s􀬿􀬵􁈻 􀵌 (-42.11±6.50, -19.09±4.37,
-1.32±0.44) and on basis of matrix elements 􀵫μ􀭧􀭨􀵯, the Velocity Ellipsoid Parameters were achieved, e.g., 􁈺λ􀬵, λ􀬵, λ􀬵; km s􀬿􀬵􁈻 􀵌
􁈺2137.36 􀵇 23.12, 6.06 􀵇 0.41, 2.53 􀵇 0.63􁈻 and 􁈺σ􀬵, σ􀬵, σ􀬵; km s􀬿􀬵􁈻 􀵌 􁈺46.23 􀵇 6.80, 2.47 􀵇 0.64, 1.59 􀵇 0.80􁈻.
For the observational quantities, we have deduced a correlation coefficient of about 􀵎 0.83 for the kinematical property of
proper motions on both sides 􁈺μ􀮑 cos δ , μ􀮔; mas yr􀬿􀬵􁈻 and the physical property with the angular distances 􁈺λ􁈻 from the
vertex, and those prove that the attributes are completely related linearly.
 
Date 2022-04-07T11:07:48Z
2022-04-07T11:07:48Z
2022-03
 
Type Article
 
Identifier 0975-0959 (Online); 0301-1208 (Print)
http://nopr.niscair.res.in/handle/123456789/59490
 
Language en
 
Publisher NIScPR-CSIR, India
 
Source IJPAP Vol.60(03) [March 2022]