50 | 8.1 | 56 5 45 | f | vF, S. 51 | 9.2 | 56 11 45 | e | eeF, eS. 52 | 9.4 | 55 56 14 | e | eeF, eS. 53 | 13.3 | 56 16 32 | f | eeF, vS. 54 | 17.6 | 56 10 33 | e | eeF, eS. 55 | 19.8 | 56 10 50 | e | eeF, eS. 56 | 23.0 | 56 11 40 | e | eF, eS. 57 | 25.1 | 56 16 43 | e | eeF, eS. 58 | 30.3 | 56 26 49 | f | eF, eS. 59 | 31.6 | 56 20 3 | e | eeF, S. 60 | 45.1 | 56 29 5 | f | eF, vS. 61 | 45.7 | 56 34 46 | e | eeF, S. 62 | 54.2 | 56 15 18 | e | eeF, eS. 63 |13 40 3.2 | 56 37 22 | e | eeF, eS. 64 | 5.9 | 56 30 56 | e | eeF, eS. 65 | 5.9 | 56 30 29 | h | eeF, 30″l. 66 | 27.2 | 56 6 27 | e | eeF, vS. 67 |13 41 27.2 | 56 20 38 | e | eF, 60″d. 68 | 38.8 | 55 47 15 | e | eF, eS. 69 | 47.4 | 55 44 54 | f | eF, vS. 70 |13 42 40.2 | 56 15 54 | e | eeF, S. ---+------------------+-----------+-----+----------------- [10] Field IV covers the position of a group of 18 small nebulae announced by E. E. Barnard in _Astronomische Nachrichten_, 125, 369, 1890. The positions there given were rough estimations from the stars B.D. +56°.1679 and B.D. +56°.1682. On the photographs, the nebulae in this region are so small and so crowded that I have been able to identify only three individuals of the group. Barnard’s Nos. 4, 7, and 18 are very probably my Nos. 41, 43, and 62. NEBULAE PREVIOUSLY KNOWN IN FIELD IV ======+==================+=============+===+=============== N.G.C.| | | | 5278 | 13ᴴ 36ᵐ 59.45ˢ |+56°18′ 3.8″ | | 5279 | 37 3.72 | 56 18 14.5 | | 5294 | 40 39.7 | 55 55 2 | f |eF, S, *15m1′np. ------+------------------+-------------+---+---------------- N.G.C. 5278 and 5279 form a double nebula, somewhat similar to Messier 51. 5278 is the nucleus and 5279 is at the tail of the arm. The spiral apparently has but one branch. TABLE XIII FIELD V OF NEBULAE