An Introduction to Modern Astrophysics · Problem 17.25

Close Binary Star Systems — Carroll & Ostlie

Physics — Astrophysics · black-holes-x-ray-binary

Problem

From the data in the text, make an estimate of the lower mass limit of the compact companion in V404 Cyg by setting the orbital inclination i=90°i = 90°. Refer to Appendix G in order to make a rough determination of the mass of the K0 IV companion. Why does your calculation result in a lower limit? What further information would be required to make a more precise determination?

Related theory

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