A Possible Orbital Solution For The Triple Star WDS 18253+4846
Bojan Novakovic
TL;DR
This paper provides orbital elements for the BC pair in the triple star system WDS 18253+4846 and analyzes the mass distribution among the components, highlighting that component C is the most massive.
Contribution
It offers new orbital parameters for the BC pair and compares mass ratios within the triple system, enhancing understanding of its structure.
Findings
Component C is the most massive in the system.
Orbital elements for the BC pair are determined for 2008-2014.
Mass ratio analysis between pairs AB and BC.
Abstract
We present here the orbital elements for the pair BC of visual binary star WDS 18253+4846 (ADS 11344 = HD 170109) and ephemerides for the period 2008-2014. As the orbital elements of pair AB already existed we analyzed mass ratio between these two pairs and concluded that components C is the biggest one in this triple system.
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Taxonomy
TopicsStellar, planetary, and galactic studies · History and Developments in Astronomy · Astronomy and Astrophysical Research