Photometric Studies of Bright Southern Binary Systems: ε Craand ψ Ori
We present results from detailed analyses of new data combined with previously published light curves of ε Cra and ψ Ori. Based on the shape of the secondary minimum of ε CrA we found that the discrepancy between the photometric and spectroscopic mass
|Collections||ANU Research Publications|
|Source:||Astrophysics and Space Science|
|01_Shobbrook_Photometric_Studies_of_Bright_2006.pdf||278.36 kB||Adobe PDF||Request a copy|
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