Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118

Fuente: arXiv
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Main Authors: Ibharalu, Elijah, Marcel, Miracle Chibuzor
Format: Preprint
Published: 2024
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author Ibharalu, Elijah
Marcel, Miracle Chibuzor
author_facet Ibharalu, Elijah
Marcel, Miracle Chibuzor
contents We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4° and separation of 3.36". Additionally, we utilized parallax and the ratio of proper motion metric (rPM) values to evaluate the potential binarity of the system. Our analysis suggests that the system may be gravitationally bound.
format Preprint
id arxiv_https___arxiv_org_abs_2403_00962
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118
Ibharalu, Elijah
Marcel, Miracle Chibuzor
Solar and Stellar Astrophysics
We present updated measurements for the position angle and separation of the double-star WDS 09168-3407 B 1118, incorporating data from our observation, Gaia Early Data Release 3 mission, and historical records. Our findings indicate a position angle of 341.4° and separation of 3.36". Additionally, we utilized parallax and the ratio of proper motion metric (rPM) values to evaluate the potential binarity of the system. Our analysis suggests that the system may be gravitationally bound.
title Astrometric Measurement of the Double-Star System WDS 09168-3407 B 1118
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2403.00962