Performance of Interference Filters in Simple Flame Photometer

1955 ◽  
Vol 27 (6) ◽  
pp. 1031-1033 ◽  
Author(s):  
W. G. Schrenk ◽  
B. L. Gendening
1988 ◽  
Vol 49 (C2) ◽  
pp. C2-105-C2-108
Author(s):  
A. MILLER ◽  
I. T. MUIRHEAD ◽  
K. L. LEWIS ◽  
J. STAROMLYNSKA ◽  
K. R. WELFORD

1963 ◽  
Vol 27 (2) ◽  
pp. 152-153 ◽  
Author(s):  
J. B. Fehrenbacher ◽  
L. P. Wilding ◽  
A. H. Beavers
Keyword(s):  

1982 ◽  
Vol 99 ◽  
pp. 121-125
Author(s):  
Philip Massey

Until now, all that we've known about the magnitudes and colors of Wolf-Rayet stars has been based on photoelectric photometry made with 50–150 A wide interference filters, selected to exclude as far as possible the stronger emission lines (Westerlund 1966; Smith 1968, Lundstrom and Stenholm 1979). This was clearly an improvement on the pioneering efforts of Pyper (1966), who obtained broad band photometry and attempted to correct for the presence of emission; nevertheless, with modern detectors it is possible to go one step further.


1983 ◽  
Vol 39 (5) ◽  
pp. 1297-1300
Author(s):  
V. A. Soglasnova ◽  
N. A. Chernyavskaya

1978 ◽  
Vol 18 (5-6) ◽  
pp. 621-625 ◽  
Author(s):  
G.D. Holah ◽  
B. Davis ◽  
N.D. Morrison

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