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 t

Details 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 t 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 t

Oct 1895

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1895an....139...17s&link_type=ejournal

Astronomische Nachrichten, volume 139, p.17

Astronomy and Astrophysics

Astronomy

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