334 PROCEEDINGS OP THE AMERICAN ACADEMY 



Remarks. 



A. New star in the nebula of Andromeda, announced by Hartwig. 



B. This star is 100 Piscium. Variation discovered by Borelly. Near a maxi- 

 mum, 1885, November 30. G. 



C. Discovered by Sawyer in 1884. Period not determined. 



D. DM. +58° 539. 



E. Discovered by Gore in 1885. 



F. The observations show a variation of about half a magnitude. The star 

 has been called T Orionis. G. 



G. Discovered by Gore in 1885. Magn. 6.15, December 13, 1885. G. 

 H. DM. +28° 1699. Sk. 



I. 60 Cancri. K. 



J. DM. +11° 1954. Variation suspected by Baxendell. K. 



K. 103 Virginis. B. 



L. This star has been called V Bootis. Max. 1885, June 1 ; magn. 72. Min. 

 1885, January 28, October 23; magn. 9.4. Computed max. 1884, September 3, 

 +266.5 E. Computed min. 1885, January 29, +266.5 E. D. 



M. Birmingham 442. Sk. 



N. Birmingham 448. Sk. 



O. Birmingham 458. Sk. 



P. Birmingham 459. Sk. 



Q. Birmingham 464. Sk. 



li. Birmingham 483. Sk. 



S. About magn. 8, 1885, August 19, September 9, November 4. G. 



T. Discovered by Gore, 1885. Confirmed by Espin and Sawyer. Variation 

 from about magn. 5.6 to 6.4. Period short, about 8^ days (G.), 8 days (Sr.). 



U. Birmingham 545. Sk. 



V. DM. +39° 4208. Found 1885, July 9, as a splendid red star, magn. 7.9, 

 since varying to 9.2; no period found; diminishing irregularly. En. Below 

 magn. 8, 1885, August 13, September 7, September 9. 



W. Birmingham 569. Discovered by Espin and confirmed by Gore. Period 

 perhaps 111± days. G. 



X. DM. +45° 3271. Sk. 



Y. DM. +45° 3289. Sk. 



Z. Discovered by Sawyer, 1885, and confirmed by Gore. Period 4.437 

 days. Sr. 



AA. Birmingham 587. Discovered by Gore, 1885, and confirmed by Sawyer. 

 Near max. 1885, January 1, August 19; near min. 1885, June 9. G. Period 

 120± days. Sr. 



BB. Variation suspected by Hind. K. 



CC. DM. +57° 2568. Fine orange red. Observed variation from magn. 

 7.0 to 8.0. Period probably short. En. 



DD. 19 Piscium. Magn. 5.5, October 3, 1885. G. 



Professor Safarik also reports the following numbers of observations 

 of suspected variable stars, which are given in the same form as in the 

 tabular statements: star in Auriga, 0,0,1; in Cants Major^ 0,0,2; in 



