The photometric orbit and apsidal motion of V526 Sagittarii

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photometry, Binary Stars, Light Curve, Stellar Orbits, Apsides, Ephemeris Time, Least Squares Method

Scientific paper

Improved photometric orbits and apsidal motion parameters are derived
from new observations of V526 Sgr (B9.5 + A2). The new orbits are
consistent with previous work on this system, but have much higher
accuracy. Further improvement in our knowledge of this system must await
completion of spectrographic work.

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