Enhanced kinematics and distribution characteristics of Upper Scorpius and Ophiuchus associations based on Gaia DR3

Fuente: arXiv
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Autor principal: Elsanhoury, W. H.
Formato: Preprint
Publicado: 2025
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author Elsanhoury, W. H.
author_facet Elsanhoury, W. H.
contents The kinematics within the Solar vicinity have revealed interesting features relevant to both stellar and Galactic structures. This study examines three stellar associations in the Upper Scorpius and Ophiuchus regions, along with their sub-samples among Gaia DR3. The calculated kinematics and velocity ellipsoid characteristics, including the mean spatial velocity components (U, V, W).
format Preprint
id arxiv_https___arxiv_org_abs_2501_10732
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Enhanced kinematics and distribution characteristics of Upper Scorpius and Ophiuchus associations based on Gaia DR3
Elsanhoury, W. H.
Solar and Stellar Astrophysics
Astrophysics of Galaxies
The kinematics within the Solar vicinity have revealed interesting features relevant to both stellar and Galactic structures. This study examines three stellar associations in the Upper Scorpius and Ophiuchus regions, along with their sub-samples among Gaia DR3. The calculated kinematics and velocity ellipsoid characteristics, including the mean spatial velocity components (U, V, W).
title Enhanced kinematics and distribution characteristics of Upper Scorpius and Ophiuchus associations based on Gaia DR3
topic Solar and Stellar Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2501.10732