Wilson and Devinney 1973
Wilson, R.E., and E.J. Devinney, 1973: Fundamental data for contact binaries: RZ Comae Berenices, RZ Tauri and AW Ursae Majoris. Astrophys. J., 182, 539-547, doi:10.1086/152162.
Differential correction analyses of three binaries of the W UMa type show that RZ Tau and AW UMa have common envelopes and the relatively small gravity darkening predicted by Lucy, while RZ Com seems to have a larger gravity effect and is only marginally in contact. Some details of our method for computing contact-binary light cruves are given. We suggest that W UMa binaries which have occultation primary eclipses may, in general, have large amplitudes for gravity darkenings or a photometric surface-brightness effect which simulates large gravity darkening.
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Wilson, R.E., and Devinney, E.J.: Fundamental data for contact binaries: RZ Comae Berenices, RZ Tauri and AW Ursae Majoris, Astrophys. J., 182, 539-547, doi:10.1086/152162, 1973.
Wilson, R.E., and E.J. Devinney (1973), Fundamental data for contact binaries: RZ Comae Berenices, RZ Tauri and AW Ursae Majoris, Astrophys. J., 182, 539-547, doi:10.1086/152162.
Wilson, R.E., and E.J. Devinney, 1973: Fundamental data for contact binaries: RZ Comae Berenices, RZ Tauri and AW Ursae Majoris. Astrophys. J., 182, 539-547, doi:10.1086/152162.
Wilson, R.E., & Devinney, E.J. 1973, Astrophys. J., 182, 539, doi:10.1086/152162.
Wilson RE, Devinney EJ. Fundamental data for contact binaries: RZ Comae Berenices, RZ Tauri and AW Ursae Majoris, Astrophys J 1973;182:539-547. doi:10.1086/152162.
R.E. Wilson, E.J. Devinney, Astrophys. J. 182, 539-547, doi:10.1086/152162 (1973).
