Long-term photometric campaign at ESO and the new eclipsing P Cygni star R 81 in the LMC

Details Long-term photometric campaign at ESO and the new eclipsing P Cygni star R 81 in the LMC Long-term photometric campaign at ESO and the new eclipsing P Cygni star R 81 in the LMC

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987msngr..47...10w&link_type=abstract

ESO Messenger (ISSN 0722-6691), March 1987, v. 47, p. 10-13.

Computer Science

3

Eclipsing Binary Stars, Molecular Clouds, Stellar Spectrophotometry, Temporal Distribution, European Space Agency, Iue, Light Curve, Spectrum Analysis, Ultraviolet Spectra

Scientific paper

The Long-term Photometry of Variables project is described. All measurements were carried out in the Stromgren uvby system and preference was given to differential measurements with two comparison stars. Included in this photometry program was the study of R 81, the counterpart of P Cyg in the LMC. A variation period of 74.59 + or - 0.01 days was obtained for this eclipsing binary.

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