G90 
PROFESSOR J. N. LOCKYER ON THE PHOTOGRAPHIC 
P 
e 
4 
X 
X 
y 
a. 
y 
/8 
Hydrse. 
8 
Herculis. 
Leonis. 
y 
Ophiuchi. 
Ursse Majoris. 
27 
Ophiuchi. 
Ursa3 Majoris. 
0 
Herculis. 
Virgin! s. 
C 
Aquilse. 
Bootis. 
29 
Cygni. 
Virginis. 
Delphini 
Bootis. 
/3 
Delphini. 
Librse. 
a 
Delphini. 
Librae. 
y 
Delphini. 
Coronae. 
Pegasi. 
Coronae. 
(2.) Tablp] B.—Stars in which there is a continuous absorption in the ultra-violet, 
extending to about K. In these stars the hydrogen lines are relatively thin. 
(a.) 
The spectra differ considerably from 
the solar spectrum, although showing a 
large number of fine dark lines. 
(dd 
The spectra have a veiy close 
resemblance to the solar spectrum. 
7 Cygni 
» 
a Cassiopeias 
p Oeti 
a Ursse Minoris 
a Arietis 
K Persei 
a Aurigae (Capella) 
/3 Geminorum 
0 Hydras 
i," H ydrae 
c Leonis 
7 Leonis 
a Ursae Majoris 
6 Virginis 
o. Bootis 
// Bootis 
e Bootis 
/3 Bootis 
c Ophiuchi 
\i Herculis 
Herculis 
!] Hercniis 
TT Hei’culis 
ft Ophiuchi 
a 0[)hiuchi 
V Ophiuchi 
7U Ophiuchi 
7 Aquilai 
r Cygni 
7 Pegasi 
// Pegasi 
