The contact binary system AH Tauri

Details The contact binary system AH Tauri The contact binary system AH Tauri

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acaps..11..143l&link_type=abstract

(Acta Astrophysica Sinica, vol. 11. no. 1, 1991) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, June 1991, p. 143

Astronomy and Astrophysics

Astrophysics

3

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, G Stars, Mass Ratios, Taurus Constellation

Scientific paper

New two-color observations of AH Tau in 1986 are given. The light curves have changed appreciably since 1973 as the new curves are symmetrical. A photometric solution is obtained using the Wilson-Devinney method. It has a degree of overcontact of 9.1 percent. The two components are found to be unevolved. The absolute dimensions are found with the help of Dworak's photometric parallax. Its distance being twice that of the Pleiades, it is probably not a member of the Pleiades cluster.

Affiliated with

Also associated with

No associations

Rating

The contact binary system AH Tauri 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 The contact binary system AH Tauri, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The contact binary system AH Tauri will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1278277