The visible universe; chapters on the origin and construction of the heavens (1892)
Gore, J. Ellard (John Ellard), 1845-1910 · London, C. Lockwood and son · leaf 188
iable as regards the actual magnitude of any individital star. Butis I have not, in my enumeration of Behrmanns stars, taken into accountrelative magnitudes, this will not influence my results. With reference togeneral stellar distribution, it is evident that Behrmanns maps are fairlyjomparable… … ■A - \ X • ■ • A- . / ■ . .w- -\.-.\ tfo
Stars · Nebular hypothesis
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