On the Galactic System With Regard to Its Structure Origin And Relations in Sp
On the Galactic System With Regard to Its Structure Origin And Relations in Sp
Karl Petrus Teodor Bohlin
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SV. VET. AKADEMIENS HANDLINGAR. HAND 43. N:O 10. 15 where in is the highest magnitude considered, N and h being functions of the lati- tude - - approximately: h=4. Oilier papers on the distribution of stars arc: A. M. Clerke. The distribution of stars, Astronomy and Astrophysics 12: 1893 pag. 515; T. W. Backhouse, The Sidereal Universe, referred to in the Monthly Notices of the Royal Astronomical Society Vol. L pag. 374; R. A. 1'roctor, Statement f views respecting the Sidereal Universe, Monthl...y Notices Vol. XXXIII. Pag. 539; J. Herschel, On the law of distribution of nebula- and clusters of stars over the surface of the heavens. Results of astronomical observations, made at the Cape of Good Hope, pag. 133. 7. Distribution of Spiral Nebulce. The attention to a certain law of distribution of the nebulae was raised by J. HERSCHEL with a statistic inquiry, by which he succeeded in pointing out two vast dominions of nebulae, each surrounding the poles of the Galaxy. This numerical sta- tement, which, according to HERSCHEL, must be considered as the expression of a real law of nature, was furthermore left unexplained.
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