686 
DR. W. HUGGINS ON THE PHOTOGRAPHIC SPECTRA OP STARS. 
with lines, as is the case in the solar spectrum. The portion of the spectrum beyond 
H is unlike the solar spectrum in character, as will be at once apparent upon an 
inspection of the map. 
Lines. 
Hi 
h 
H 2 
Of. 
W. L. 
4340 
4325 
4307-5 
4289 
4271 
4252-5 
4237-5 
4227-5 
4214 
4201 
4195 
4185 
4176 
4170 
41501 
4141 J 
4132-5 
4112 
4099 
4075 
4064 
4055 
4045 
4034 
4040 
3995 
3980 
3968 
3933 
3920 
3905 
3900 
3887-5 
3881 
3870 
3859 
3856 
3850 
3838 
3835 
3832-5 
as in solar spectrum, 
doubtless the group G 
clearly multiple. 
stronger. 
thin. 
probable group, 
thin rather. 
W. L. 
« 3822-5 
3815 
3814-5 
3810 
3805 
3798 
7 3795 
3789 
3775 
3762-5 
3755 
6 3745-5 
3732-5 
£ 3730 
v 3717-5 
e 3707-5 
3702-5 
3690 
3682-5 
3672-5 
3662-5 
3657-5 
3641 
3637-5 
3625 
3610 
3602-5 
3592-5 
3585 
3575 
3560 
3551 
3515 
3507-5 
3504-5 
3487 
3482 
3475 
3467 
3457 
