V1507 Cygni (HD187399): A Highly Evolved, Enigmatic Interacting Binary System with an Eccentric Orbit
T. J. Davidge

TL;DR
This study analyzes the properties and evolution of the eccentric binary system V1507 Cyg, revealing its stable period, mass transfer history, and the nature of its components through spectral analysis and environmental context.
Contribution
It provides detailed spectral and dynamical analysis of V1507 Cyg, including component masses, orbital stability, and evolutionary state, highlighting its complex mass transfer history and environmental interactions.
Findings
Component masses: 6.4 and 14.0 solar masses
Stable orbital period over decades
Eccentric orbit likely due to hierarchical evolution
Abstract
The properties of the interacting, eccentric orbit binary V1507 Cyg (HD187399) are examined with spectra that cover wavelengths from 0.63 to 0.68um. The spectrum of the brightest star is very similar to that of the B8 I star Beta Ori, although with absorption lines that show sub-structure consistent with a varying tidal field. The bulk of the Halpha emission in the spectrum appears to be associated with the brighter star. Evidence is presented that the period of the system has been stable over timescales of many decades, arguing against large-scale mass transfer at the current epoch. Absorption and emission lines are identified that originate in an expanding asymmetric envelope around the companion, and component masses of 6.4 +/- 0.9 and 14.0 +/- 0.9 solar are found, where the former applies to the brighter star and an inclination of 46 degrees has been assumed. The evolutionary state…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
