New Observations and Analysis of the Bright Semi-Detached Eclipsing Binary mu1 Sco

Details New Observations and Analysis of the Bright Semi-Detached Eclipsing Binary mu1 Sco New Observations and Analysis of the Bright Semi-Detached Eclipsing Binary mu1 Sco

2009-10-07

arxiv.org/abs/0910.1241v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 figures, 6 tables, 9 pages, uses mn2e.sty, to be published in MNRAS

Scientific paper

Using new and published photometric observations of mu1 Sco (HR 6247), spanning 70 years, a period of 1.4462700(5) days was determined. It was found that the epoch of primary minimum suggested by Shobbrook at HJD 2449534.178 requires an adjustment to HJD 2449534.17700(9) to align all the available photometric datasets. Using the resulting combined-data light-curve, radial velocities derived from IUE data and the modelling software PHOEBE, a new system solution for this binary was obtained. It appears that the secondary is close to, or just filling, its Roche-lobe.

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