Science: v.1-v.219Moses King, 1969 |
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Page 811
... spectra agrees with the corresponding averaged spectrum obtained on another night , and they are significantly different from each other . The circularly polarized spectra are fairly uniform over the fre- quency band that we observed ...
... spectra agrees with the corresponding averaged spectrum obtained on another night , and they are significantly different from each other . The circularly polarized spectra are fairly uniform over the fre- quency band that we observed ...
Page 1055
... Spectra , Variability , Size , and Polarization of H2O Microwave Emission Sources in the Galaxy Abstract . Radio ... spectra were measured with a bank of 50 contigu- ous filters , each 4 khz wide . Since the source spectra were ...
... Spectra , Variability , Size , and Polarization of H2O Microwave Emission Sources in the Galaxy Abstract . Radio ... spectra were measured with a bank of 50 contigu- ous filters , each 4 khz wide . Since the source spectra were ...
Page 1056
... spectra of the W49 and Orion source regions , which were measured with a resolution of 4 khz , are shown in Figs . 1 and 2. Both have a number of sharp , Doppler - shifted lines with some line widths as narrow as 0.6 km / sec and some ...
... spectra of the W49 and Orion source regions , which were measured with a resolution of 4 khz , are shown in Figs . 1 and 2. Both have a number of sharp , Doppler - shifted lines with some line widths as narrow as 0.6 km / sec and some ...
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