Two bright eclipsing binaries solved with the help of visual observations

Details Two bright eclipsing binaries solved with the help of visual observations Two bright eclipsing binaries solved with the help of visual observations

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007oejv...68....1o&link_type=abstract

Open European Journal on Variable Stars, vol. 0068, Issue 1, p.1

Computer Science

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Visual observations of V975 Cen and NSV 15737 were combined with photometric data from the Hipparcos and ASAS databases to determine the elements for these eclipsing binaries. V975 Cen is an Am+F binary in an extremely eccentric orbit with elements HJD 2454217.582 (±0.080) + 135.9255 (±0.0015) x E. NSV 15737 is an EA-system made up of very different components with elements HJD 2454329.479 (±0.001) + 8.161235 (±0.000001) x E.

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