Gore— ^ Revised Catalogue of Variable Stars. 125 
^0. 24 a. E Reticuli. — Discovered in 1867, at the Madras Obser- 
vatory by the Hindoo observer, Eagoonatha Chary, but not included 
in any Catalogue of variable stars hitherto published. 
'No. 29. e Auriga. — Schmidt, in 1883, found the fluctuations of 
light very small. The maximum and minimum given in the Catalogue 
were observed by Sawyer, who found a variation of about ^ a magni- 
tude in 1884. My own observations, 1875-1885, show a variation of 
about ^ a magnitude. 
No. 30. E Lepoeis. — The maximum given was observed by Sawyer 
(mag. 5-7). 
No. 32. E Atieig^. — A maximum observed by Schmidt, 1883, 
January 30*0 (mag. 7'8). Increase of light quicker than the decrease. 
A minimum, 1883, K'ovember 3 (mag. 9-2) {A. iV., 2577). Espin finds 
that the bright bands of the spectrum are brighter as the star is on the 
increase, and fainter as it decreases. 
No. 33. S AuEiG^. — Maximum observed by Duner. 
1^0. 34. S Ohionis. — Maximum observed by Knott. 
No. S4a. 31.0eionis. — My observations from JS^ovember, 1884, to 
February, 1887, show only a small variation — 5-0 to 5*5, with appa- 
rently no regular period. 
No. 35. S Oeionis. — Sawyer found the light of this star constant 
from January 2 to April 10, 1883, and he could not detect the least 
sign of variation " from IS'ovember, 1884, to February, 1885. 
No. 36. T Oeiokis. — My observations of this star from January, 
1885, to February, 1887, show a variation of about half a magnitude. 
It is a double star, 0^ 111. 
No. 36 a. — Oeionis. — No. 822 of Bond's Catalogue of Stars in 
the great nebula in Orion. It was independently discovered to be 
variable by Schmidt, in April, 1878, and by Common, in 1883, by 
means of photography. It is No. 161 of my Catalogue of Suspected 
Variables. 
37 a. U ('* KovA ") Oeionis.— Found by me with a binocular field- 
glass, 1885, December 13, 9^20™ (Dublin, M. T.), as a reddish star of 
