A calculation of structural parameters of spherical stellar systems by means of characteristic functions method. I. Theory

Theory of the determination, by means of

Theory of the determination, by means of a single spectroscopic observation, of the absolute dimensions, masses and parallaxes of stellar systems whose orbits are known from micrometrical measurement; with a rigorous method for testing the universality of the law of gravitation

✍ T. J. J. See 📂 Article 📅 1896 🏛 John Wiley and Sons 🌐 English ⚖ 442 KB 👁 2 views

Band 139. N! 3314. Theory of the determination, by means of a single spectroscopic obHervation, known from micrometrical measurement ; with a rigorous method for testling the universality of the law of gravitation. of the absolute dimensions, masses and parallaxes of stellar systems whose orbits