Eclipsing binary UW Bootis

Details Eclipsing binary UW Bootis Eclipsing binary UW Bootis

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.133..291s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 133, no. 2, 1987, p. 291-296.

Astronomy and Astrophysics

Astrophysics

1

Eclipsing Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Light Curve, Periodic Variations, Stellar Magnitude

Scientific paper

Photometric observations of UW Bootis in U, B, and V filters are analyzed and compared with the data of Gaposchkin (1939). Examination of the light curve reveals that the primary minimum is symmetrical and its depth is 0.66 mag in all three filters. The total duration of the eclipse is 0.20 P. The mean value of time minima in U, B, and V filters was determined using the Kwee and Van Woerden (1956) method, and O-C values were calculated using the ephemeris. It is concluded that the period of UW Boo is constant, and no oscillations of the primary minimum with a period of ten years are detected.

Affiliated with

Also associated with

No associations

Rating

Eclipsing binary UW Bootis does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Eclipsing binary UW Bootis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Eclipsing binary UW Bootis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-856735