Gore — A Revised Catalogue of Variable Stars. 
12a 
:No. 65. V Cassiopeia = DM 47°, 194. Observed 8-5 m. by Espin, 
1886, JSTovember 30 ; on February 6, 1887, it was only 9-9 ; on Te- 
bruary 20, ll'O, and on Marcli 13 it had faded to 13*0 m. The 
variability has been confirmed by Baxendell. 
No. 7. U Cephei. — Minima of this remarkable variable were ob- 
served by Baxendell, 1885, March 9, 9M3™-5 (9-4 m.); and 1885, 
August 3, lP53™-5 (9-3 m.); by Baxendell, junior, 1885, August 3, 
IP 51™ (9-3m.) ; and by Knott, 1885, March 14, 9^ 32™ G.M.T., and 
March 19, 9^ 12- G.M.T. 
No. 9 a. — PisciuM. — Found to be variable by C. H. F. Peters, from 
observations at Clinton, U.S.A. (1879-1880); he found it 10 m. on 
January 5, 1880, but on other occasions much fainter, and sometimes 
invisible Later observations gave a period of 330 or ^-^^days. 
No. 11. E PisciTJM. — Duner and Vogel find a spectrum of the third 
type with very large and dark bands. Maxima were observed by 
Schmidt, 1881, December 18 (mag. 7) ; 1882, December 5-3 (mag. 8), 
{Asf. Nad., 2491); and 1883, Nov., 17-5) (mag. 7-5). {A. N., 2577). 
No. 13. E Aeietis. — Maxima were observed by Baxendell, 1884, 
August 3 (mag. 8*1), and 1885, February 3 (mag. 9*0), the lowest 
maximum magnitude" he had ever observed in this star. {Observatory, 
April, 1886.) 
No. 14. o (Miea) Ceti. — The following are observed maxima since 
1882:— 
Year. 
Date of Max. 
Brightness. 
Observer. 
Remarks. 
1884 
March 6 (?), 
4-6 
Sawyer, 
1 1 or 2 steps brighter than 
\ K Ceti. 
1885 
February 4, 
2-7 
Gore, 
1885 
< 
February 10, 
2-7 
Sawyer, 
4 steps less than a Ceti. 
1885 
February 11, 
2-9 
Knott, 
1885 
February 14, 
2-6 
Baxendell, 
1885 
December 22, 
4-9 
Gore. 
1885 
Deceruber 29 to \ 
{ Jan. 13, 1886, ] 
4-5 
Numsen. 
1886 
November 20 (?), 
4-3 
Gore. 
1886 
November 30, 
4-05 
Markwick. 
1886 
December 30, 
4-4 
Sawyer. 
