132 Proceedings of the Royal Irish Academy. 
]N"o. 96 l. 34 EooTis. — Schmidt deduced a period of 361 days, with 
a maximum, 1876, Pebruary 24, and with remarkable anomalies in 
the light curve. The variability was confirmed by Schwab. 
IN"©. 96 c. U Boons. — Maximum and minimum given were ob- 
served by Baxendell ; max. mag. 9*5. {Olservatory, April, 1886.) 
1^0. 98. T Trian. Austealis. — Observations of this and other 
southern variables are much required. 
]S"o. 103. S CoEON^. — The following maxima have been observed 
in recent years : — 
1882, May 10, 7-7 mag. Schmidt. 
I 1883, May 1-5 7-6 „ Schmidt. 
( 1883, May 3, 7'3 ,, Sawyer. 
I 1884, April 30, 6-6 „ Baxendell. 
( 1884, May 5, 7-3 „ Sawyer. 
1885, May 8, 7-6 Baxendell. 
Baxendell, from observed maxima, 1864-1884, deduces a mean 
period of 360*416 days, with Epoch, 1873, June 27-0. The rise from 
minimum to maximum occupying about 126 days, and the fall from 
maximum to minimum about 234 days. Sawyer also finds the 
increase of light rapid, and the decrease slow. {A.JV., 2591.) 
1^0. 106 LiBE^. — Period somewhat irregular, but less than one 
year, according to Peters {private letter, 1885). 
'^0. 107. E CoEON^. Schmidt observed a minimum of 12 m. about 
the middle of August, 1883 {A. JV., 2577) ; and Sawyer a minimum of 
7-4, 1885, October 13. 
ITo. 108. ESeepentis — Knott observed this star at the mag. 11-5, 
on April 20, 1885. 
Ko. 109. Y CoEON^. — Maxima of this star have been observed as 
follows : — 
1878, October 5, Duner. 
1879, October 12, Schmidt. 
1881, October 3, Schmidt. 
1882, September 16, Schmidt. 
1883, September 24, Chandler. 
1883, September 5, Schmidt. 
1885, August — , Duner. 
