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The stars B Aurigae A and B Aurigae B constitute a double-lined spectroscopic binary with an orbital period P = 3.96 days. The radial
The stars B Aurigae A and B Aurigae B constitute a double-lined spectroscopic binary with an orbital period P = 3.96 days. The radial velocity curves of the two stars have amplitudes vA sin i = 108 kms- and vg sin i = 111 km s-1. If i = 90, what are the masses of the two stars? %3D %3D
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Physics
Authors: David Young, Shane Stadler
10th edition
1118486897, 978-1118836873, 1118836871, 978-1118899205, 1118899202, 978-1118486894
