€ 
e 
273 
THE SPECTRUM OF NOVA PERSEI AND THE STRUCTURE OF ITS BANDS. 
TABLE X. 
Residuals, 
elisa 1S esc Pe sess fl ieee se) ih ee sea) sed 
oooo 
ae arse Nt fee Seah ae apse ab Sesh yj Sb Sb SR 
Oe =) 
aes as 
+ 1+ Te ease Ieee epee Wy Se et pS ae y 
b=1'4. 
(17) 
by Formule (7) and (11). 
D=i1-08: 
SY DMASCSOHMANTAIEARAODODOCNDANROONMHHANHODWDOCONDH 
SSHKLOROLORSOSCHHDRDERRDOSOSOSHOHAANNHAAG 
a4 mr are CD on en ee De 
i aS 
U we 
i! 
er St 
Oy — wz 
Mo. 
FH+tH+HtHe+tHttettettette¢ttte+¢te+eesge 
Val Sr ek ibirlistil 
No. 4. 
2m. 
AOOMArEEDARBDOCOCODDNDDAGAMrDODrAOONMDNSO 
reali! al Se 
Veet iso\ Leal Lael tl eat! 
Me. 
6 00 OD I~ 10 10 69 1 lezeuees | 
Ms. 
SOHHMMNNHO Ic = 
HOSOHMOOMIOW | HOr~AK HOMO 
SAAAN To HO 
My. 
SOSDDDD tw MN OD D> 0016190 HOMm~NM~ OCOOM 1G 
SOnNNDNATHO SHANNA WWwHA KG 
Superposed Bands. 
| 
Ms. 
Mo, 
Ho3 0 1d LO conon ro) 
ep ere N 
Intensity Curves of the different 
Calculated Intensity Curves, Xm and (m), for Photographic Plate 
My. 
Sy SUemiwgl tsa ten: (saecwa sill) Gl karesy elk Neste) seri of. eee SND HHCDORM 
SOO nTtNANMNG SOnnAMtAHOAN GH 
=0 
*G + Sysuaq uy pearesyQ 
na 1 Pe eS 
ADMWONMKRKRKRDADOHOCSCODBMAARDDADOCDHMONH 
} af Stn Coma ET a | rt 
