Gore — A Revised Catalogue of Variable Stars. 
133 
Chandler gives tlie following elements : — 
Max. = 1878, October 13-3 + 359-5 E. 
Dimer gives 
Max. = 1878, October 21-7 + 356-52E, 
and 
Min. = 1879, May 3 + 356-52 E. 
jN'o. 109 a. — Lupi. — Discovered to be variable at Cordoba in the 
course of the observations for the Cordoba Zone Catalogue. 
'Ho. llOa. — LiBE^. — Discovered to be variable by Professor Peters, 
at Clinton, U.S.A., in 1885. It was observed as 8^ m. at Markree, 
on May 8, 1851 {private letter, July, 1885). 
IS'o. 114. — ScoEPii. — Maximum given was observed by Schmidt, 
mag. 12. 
1^0. 116. E ScoEPii. — The following recent maxima have been 
observed : — 
1882, April 24*2, lO'O mag. Schmidt. 
( 1883, July 9, 10-1 „ Knott. 
I 1883, July 11-5, 10-3 „ Schmidt. 
1885, May — , — — Knott. 
1886, July 28, — — Knott. 
!N"o. 117. S ScoEPii. — Maxima were observed by Schmidt, 1882, 
May, 29-3 (10-5 m.) ; and 1883, May, 14-5 (10-5 m.) 
]S"o. lis a. — Ophiuchi.— This is Birmingham, 379; Birmingham's 
observations, 1873-1876, vary from 7-5 to 9-9-5. Duner observed a 
maximum in 1885, about end of March. 
E'o. 119. U Herculis. — A. maximum was observed by Baxendell, 
1885, July 14 (mag. 7-4). 
1^0. 121. (30) Heeculis. — In 1882 Schmidt found a mean period 
of 91 days ; Sawyer, in 1885, found periods of 59 to 75 days from 
observations of maxima, and about 68 days from the minima. 
1^0. 124. — Heectjlis = DM 37°, 2771. — Duner observed a maxi- 
mum in September, 1885. He finds a spectrum of the third type with 
the bands strongly developed in the ultra blue, but feeble in the red. 
