Investigation of the spectral content of a cw CO laser output using a high-resolution scanning Fabry-Perot interferometer

1976 ◽  
Vol 8 (5) ◽  
pp. 221-226 ◽  
Author(s):  
R.B. Dennis ◽  
H.A. Mackenzie ◽  
G. McClelland ◽  
F.H. Hamza
2015 ◽  
Vol 35 (6) ◽  
pp. 0630007
Author(s):  
柳文娟 Liu Wenjuan ◽  
胡澄之 Hu Chengzhi ◽  
姜培培 Jiang Peipei ◽  
吴波 Wu Bo ◽  
沈永行 Shen Yonghang

2018 ◽  
Vol 16 (11) ◽  
pp. 110603 ◽  
Author(s):  
Peng Cui Peng Cui ◽  
Wentao Zhang Wentao Zhang ◽  
Ying Song Ying Song

1989 ◽  
Vol 131 ◽  
pp. 200-200
Author(s):  
K. C. Sahu ◽  
S. R. Pottasch ◽  
B. G. Anandarao ◽  
J. N. Desai

Kinematic study of the multiple shell PN NGC 3242 was carried out by obtaining Hα and [O III] line profiles at 9 positions of the nebula using a high-resolution (R ≅ 50,000) Fabry-Pérot spectrometer. The positions cover both the bright inner shell and the faint outer shell. It is shown here that the two apparently continuous shells are kinematically separate: the faint outer shell was ejected ∼ 5000 years earlier and has less expansion velocity than the bright inner shell.


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