The Nature of the Bright Early-Type Eclipsing Binary Theta 1 Ori A = V1016 Orionis

Computer Science

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Early-Type, Eclipsing Binary, Pre-Main-Sequence

Scientific paper

Analysis of the published photometry of theta 1 Ori A yields an improved
ephemeris of JD 2442752.022(+/-0.004) + 65.43280(+/-0.00008)xE.
Modelling the light curve suggests that the primary component is a early
B-type main-sequence star and the secondary is a pre- main-sequence star
about spectral type A0.

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