Taurus stars membership in Pleiades open cluster
A. L. Tadross, M. A. Hanna, N. S. Awadalla

TL;DR
This study analyzes the properties of the Pleiades open cluster using near-infrared data, comparing it with optical observations, and examines the membership of variable binary stars in Taurus in relation to the cluster.
Contribution
It provides new insights into the membership and characteristics of stars in the Pleiades cluster using infrared data and compares these with optical observations.
Findings
Membership validation of variable binary stars in Taurus.
Comparison of infrared and optical data for Pleiades.
Insights into physical properties of Pleiades stars.
Abstract
In this paper, we study the characteristics and physical properties of the young open cluster Pleiades (NGC 1432; M45; Melotte 22; Seven Sisters) using Near Infra Red, JHK pass bands. Our results have been compared with those found in optical, UBV, newly observations. The membership validity of some variable binary stars, which are Located in Taurus constellation, and their relation with Pleiades cluster have been achieved.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research
