Possible evidence for gravitational Bohr orbits in double galaxies - The Peterson, Turner, and Karachentsev samples

Details Possible evidence for gravitational Bohr orbits in double galaxies - The Peterson, Turner, and Karachentsev samples Possible evidence for gravitational Bohr orbits in double galaxies - The Peterson, Turner, and Karachentsev samples

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.126..185d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 126, no. 1, Oct. 1986, p. 185-191.

Astronomy and Astrophysics

Astrophysics

1

Bohr Theory, Celestial Mechanics, Galaxies, Gravitation Theory, Orbital Mechanics, Circular Orbits, Distribution Functions, Plancks Constant

Scientific paper

A phenomenological model of double galaxy dynamics is constructed, assuming a Bohr model for isolated point galaxies bound together in circular orbits by the Newtonian gravitational force. The model is tested by using experimental data from three independent random samples of isolated pairs. In each case, the data provides cautious support for the existence of gravitational Bohr orbits in double galaxies, with a mean cosmic Planck's constant/2 pi given by about 5 x 10 to the 74 the erg s.

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