21(3 
SIR NORMAX LOCKYER AXD .MR. F. E. BAXANDALL 
Wave-lengths, Intensities, and Probable Origins of y Cygni Lines, compared with 
those of S Oaiiis Majoris, the Chromosphere, and a Cygni— continued. 
7 Cygni 
5 Cauis majoris 
Chromosphere 
(Jvensingbon). 
(llaryard). 
(Kensington). 
Inten- 
A of 
probable 
i Inten- 
Inten- 
A. 
sity. 
Mas. 
Probable 
origin. 
A. 
sity. 
Mas. 
A. 
sity. 
Mas. 
= 10. 
origin. 
1 = 220. 
= 10. 
1134 -8 
3-4 
Fe 
4134 -84 
413 t-8 
8 
4134 -8 
3 
36-9 
5 
/ Fe 
1 Fe 
36-68 
37 -16 
1 -- 
— 
— 
— 
} 37-4 
3 
37 -0 
3 
3 7 -9 
5 
Fe 
37 -81 
J - 
_ 
_ 
_ 
40 -1 
3 . 
Fe 
40 -09 
_ 
40 -1 
1 
42 -3 
3 
/ Fe 
1 Cr 
42 -03 
42 -33 
} - 
— 
42 -3 
1 
43 -8 
8 
f Fe 
1 Fe 
43 -57 
44 -04 
1 43 -9 
5 
43 -8 
5-6 
4-! ■ 0 
2-3 
Fe 
46 -23 
— 
46 -0 
1 
■ill '7 
3 
/ Mn 
1 Fe 
47 '65 
47 -84 
} - 
— 
47 -5 
1 
49 -4 
5-6 
Fe 
49 -53 
49 -5 
0 
49 -4 
3-4 
50 - I 
1 
— 
— 
_ 
_ 
_ 
52 -3 
3 
Fe 
52 -34 
— 
— 
52-1 
2 
r 5 4-07 
1 
54 ’5 
5 
Pc 
54-67 
[ 54-98 
1 51-9 
2 
5 1 -8 
2-3 
56 7 
6 
— 
— 
56 -7 
2 
56 -5 
3 
57 "9 
1 
Fe 
57 '05 
— 
— 
57 -8 
1 
59 -2 
3 
f Fe 
t Un 
r 58 -96 
1 59 -35 
} - 
— 
58-9 
1 
60 "5 
3 
_ 
61 7 
6-7 
7' '-Ti 
61 -68 
61-7 
3 
61-7 
3 
63 ’8 
5 6 
p Ti 
63 -82 
63 -9 
2 
63 -8 
4 
65 '5 
3 4 
Fe 
65 -55 
— 
— 
— 
1 
67 '6 
3-4 
— 
— 1 
67 -5 
1 
67 -5 
1 
2-3 
1 
71 -2 
1-2 
/ Fe 
1 P Ti 
71 -07 
71-21 1 
} ” 
— 
— 
— 
72 -1 
3-4 
p Ti 
72-07 
— 
72-1 
3-4 
73 ’6 
4-5 
r p Fe 
1 P Ti 
73 -52 
73 -70 
72 *0 
73 '6 
Il3 
73 -5 
4-0 
75 *4 
1 
_ 
_ 
— 
77 7 
4 
P Y 
77 -75 
77 -8 
3 
77 
5 
79 -0 
5 
pi Fe 
78-95 
79 -5 
4 
79 -0 
4-5 
81 -9 
4-5 
Fe 
81 -92 
82 -0 
1 
81 -9 
3 
84-5 
5 
P Ti 
84-40 ' 
85 -0 
2 
84-6 
2-3 
87 -2 
f Fe 
87 -20 
1 87 -6 
87-6 
87 -8 
I*" 
1 Fe 
87-94 1 
4 
4-5 
90 7 
1 
— 
- 1 
_ 
_ 
_ 
91 7 
5 
J Fe 
1 Fe 
91 -59 
91 -84 
1 91 -8 
3 
91-7 
3 - 4 . 
93-4 
1 
— 
_ 
_ 
_ 
95 '5 
4 
Fe 
95 -49 
— 
— 
95 "5 
1 
a Cvgni 
(Kensington). 
double. 
4138 -4 1 
43 -9 
46 -0 
49 7 
61 7 
63 -0 
63 -3 
67 -6 
72 -0 
73 -5 
77 -8 
79 -0 
81 -8 
85 -0 
88 -0 
92-0 
1-2 
2 
<1 
1-2 
<1 
3-1 
69-8 <1 
2-3 
6 7 
2-3 
6-7 
<1 
<1 
? double. 
'Bi’oad, probably 
compounded of 
tlie tli:ee solar- 
Fe lines. 
'Probably identi¬ 
cal witb un¬ 
known solar 
line 4156 '47. 
'Un = strong solar 
line, to wbicli 
Rowland as¬ 
signs no origin 
f Probably identi¬ 
cal with strong 
I solar line 
1 4167 '44, to 
I which Kow- 
I LAND assigns 
I no origin. 
Probably close 
double. 
? double. 
Close double. 
