Jones, H. Spencer (Harold Spencer), 1890- · London E. Arnold & co. · leaf 402
-10 „ -30 •154 6^07 672 -30 „ -50 •129 3-71 261 -50 „ -70 •124 3-21 154 -70 „ -90 •125 3-14 111 The values in the last column are derived from Herschels star gauges, or counts of stars visible in a definite area inthe field of his 18-inch reflector. From this table it will be seen that the… … Tiiii L \i;iM-, .M,\i:i;i i an ic ( i.iiim) THE STELLAR UNIVERSE 353 and form part of it or are in some way definitely connectedwith it. Down to a limit of the ninth magnitude, the starsare nearly three times as dense in the Milky Way as at thegalactic poles, whilst for the stars of Herschels…
Astronomy
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