Contact and near-contact binary systems - III. The semi-detached system YY Ceti
T. M. McFarlane, David King, R. W. Hilditch
Abstract
Open-access reader
T. M. McFarlane, David King, R. W. Hilditch
Abstract
Open-access reader
Reticon spectroscopy and BVRIc photometry are presented for the eclipsing binary system YY Ceti. It is shown that the system, which has an orbital period of 0.79 day, is composed of a normal main-sequence star of spectral type A8 and an evolved late G-type secondary which completely fills its Roche lobe. The system is expected to evolve into contact within |$\sim {10}^{9}$|yr.
OpenAlex reports 10 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Reticon spectroscopy and BVRIc photometry are presented for the eclipsing binary system YY Ceti. It is shown that the system, which has an orbital period of 0.79 day, is composed of a normal main-sequence star of spectral type A8 and an evolved late G-type secondary which completely fills its Roche lobe. The system is expected to evolve into contact within |$\sim {10}^{9}$|yr.
Key concepts: Physics, Contact binary, Roche lobe, Photometry (optics), Astrophysics, Orbital period, Contact system, Binary system