TY  - JOUR
T1  - Concise Rules for Computing the Effects of Refraction and Parallax in Varying the Apparent Distance of the Moon from the Sun or a Star; Also an Easy Rule of Approximation for Computing the Distance of the Moon from a Star, the Longitudes and Latitudes of Both Being Given, with Demonstrations of the Same: By the Rev. Nevil Maskelyne, A. M. Fellow of Trinity College, in the University of Cambridge, and F. R. S.
JF  - Philosophical Transactions (1683-1775)
VL  - 54
SP  - 263
EP  - 276
PY  - 1764/01/01/
UR  - http://dx.doi.org/10.1098/rstl.1764.0046
M3  - doi:10.1098/rstl.1764.0046
AU  - Maskelyne, N.
ER  -