Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1779064 | New Astronomy | 2013 | 6 Pages |
Abstract
⺠We determined the nature and structures of HH Boo. ⺠We obtained multi-colour light curves. ⺠We analysed the orbital period variation. ⺠There is mass transfer from the second component to the primary. ⺠We demonstrated that HH Boo should be an A-type W UMa binaries.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
H.A. Dal, E. Sipahi,