1 
(XXXIV)] NEBST EINER UNTERSUCHUNG ÜBER SYSTEMATISCHE FEHLER. 459 
Bemerkungen. 
Epoche. 
Sternzeit. 
Vergr 
Temp. 
Distanz 
Refraction 
Positionsw. 
Refraction 
Bilder. 
2.2104.— 8 Delphini. (A=3.5; B=4.5; C—11.0) 
a — 20^32"4 ۵ — + 14913' 
AA B u. C. 
2 
1890.6 |21^26»! TIT| 4-1020 | 36712 | 4- 07017 1832043’ | + 0/7 | 2—8 
1890.6 ۱20 2 |III| +11.7| 35.69 | + 0.019 1332 51 |+ 0.2/8 | 
1890.8 |21 21 | III| — 0.2 36.36 | 0.017 1333 6 |+07|4 
Fadenbeleuchtung. 
1891.0| 1 27 |III| — 5.9| 36.53 | + 0.030 |382 26 |+4.9|4 | 
1890.8 | 36.175 ~- 0.021 2 46.5 + 1.6] 
0.2. 410. (4264; B= 6.7; C= 7.7) 
a = 20^35"6 8 — + 40011’ 
A+Bu. C. 
2 
1889.9 123 20 | II | + 3 68.82 | 4- 0.024 | 69 32 0.0۱1 — | Unsichere Beob. Ne bel 
1889.9 | 1 18 || —11.8| 68.23 |--0.042| 69 29 | +0.2 8—4| Objectiv bereift. Gew. 0.5 
1891.01 0 43 | II | — 9.0] 68.22 | 4-0.031| 69 40 | 4-0.1|4 
1891.1| 5 12 | m | — 3.7| 68.57 | به‎ 0.082| 69 46 | — 8.1|8—4 
1891.8 |14 52 | III! + 0.9| 68.39 | 4-0.045| 69 36 | —1,7|2—8 
1890.7 | | 68.853 + 0.047 69 37.11 — 1.0 
0.2. 461.—15 Cephei. (A=5.9; B—10.6; C=9.5) - 
&—92^0 7 A — + 59019’ 
A u. C. 
1890.018 3 ۱1] | - 5.8| 88.95 | + 0.037 | 39 9 |= 0.2 | 3—4 
1890.1 | 2 53 | II | — 0.6 | 89.29 |+ 0.036 | 38 58 |+0.4|2—3 
18902 | 5 33 | II | — 5.1 | 89.30 | + 0.060| 38 50 | 0.9 | 4 
1891115 8 | II|— 2.1| 88.81 | + 0.058| 39 5 |+0.7|3 
1891.1 | 5 30 | II | — 8.71 89.19 | + 0.058| 38 55 -+ 0.7 | 3—5 
1890.5 89,108! + 0.050 | 38 59,4 + 0.6 
Mélanges mathém. et astron. T. VII, p. 217. 
