COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 713 Konkoly Observatory Budapest 1972 September 11 OBSERVATIONS OF THE EXTREMELY YOUNG STELLAR GROUP Lk H-alpha 224 AND 225 The evolutionary significance of the stellar group near BD + 40d4124 was first noticed by Herbig (ApJ Supp. 4, p.337). Later Cohen (ApJ 173. L 61) and Strom et al. (ApJ 173, L 65) detected large infrared excesses of members of the group. Furthermore the data of Strom et al. revealed some optical variability of Lk H_alpha 225 and of BD + 40d4124 itself. Though the remark of Strom et al. on the strong variability of Lk H_alpha 225 seemed not to be conclusive, as they compared the red photograph of Herbig (l.c.) with their own blue plates. a private communication of Dr. Herbig satisfied the doubts. I estimated the stars Lk H_alpha 224 and 225 on Sonneberg plates with the following results: Lk H_alpha 224 is more often bright than faint. In maximum light there are irregular fluctuations generally between 13.0m and 14.0m (cycle length roughly 50 days) which occasionally are interrupted or terminated by minima (extreme case: 17.3m) lasting days or weeks. Total range: 12.6m to 17.3m pg. Lk H_alpha 225 is usually fainter than 16.5m and invisible on the majority of plates, A series of Heidelberg 40 cm astrographic plates from 1958 April to July shows the star irregularly varying between 17.0m and 17.8m near the plate limit. On the POSS prints the object is about 16.8m (O 754) and 17.8m (O 1145), Strom et al. measured B = 18.2 (1971 Oct. 14). The outstanding fact is that two eruptions are observed: 1962 June 2, Oct.4 15.4m (May 31 fainter than 16.0m), 1963 Sep. 13 15.7 (isolated plate). Total range: 15.4m to 18.2m pg. W. WENZEL Sternwarte Sonneberg DDR-64