The paper discusses the advantages of fused silica etalons in hyperfine structure analysis of spectral lines. It is shown that the temperature effect on the patterns produced by such plates is negligible as compared with that on patterns from Lummer plates either of quartz or of glass. Long exposures in photographing the patterns are thus rendered possible. The re-examination by the authors of a few prominent lines of mercury using these etalons has revealed faint satellites not previously recorded. A microphotogram showing a new satellite at −0.154 Å. for HgI 5461 Å. is here reproduced
Hyperfine structure lines of highly-charged ions may open a new window in observations of hot rarefi...
We have applied the technique of speckle masking to spectra. The obser- vation of elongated solar s...
The primary objective of this program was to obtain FUSE observations of the multiple interstellar a...
The paper discusses the advantages of fused silica etalons in hyperfine structure analysis of spectr...
Spectral lines, widths, and shapes are powerful tools for emitting/absorbing gas diagnostics in diff...
We present CLOUDY calculations for the intensity of coronal hyperfine lines in various environments....
Optically excited mercury resonance radiation was used as a light source to provide the sharpest pos...
Spectroscopic methods of measurement of high temperatures are reviewed briefly. They refer mostly to...
We have used H band spectra from IGRINS (R ~45000) of 34 K giants to investigate the limits of infra...
Author Institution: Theoretical Division, T-4 MS B212, Los Alamos National Laboratory; NASA - Goddar...
The hyperfine structure of mercury extracted from neutron irradiated gold has been investigated with...
SUMMARY: Taking into account effects of hyperfine structure, we calculated the synthetic solar spect...
Abstract. We have analysed the 10 m spectral region of a sample of Herbig Ae/Be (HAEBE) stars. The s...
[1] Ch. Salomon, Ch. Breant, Ch. Borde and R.L. Barger J. Physique Colloques 42 C8 (1981) [2] A. Cla...
There are several problems in astrophysics that cannot be addressed until very high resolution spec-...
Hyperfine structure lines of highly-charged ions may open a new window in observations of hot rarefi...
We have applied the technique of speckle masking to spectra. The obser- vation of elongated solar s...
The primary objective of this program was to obtain FUSE observations of the multiple interstellar a...
The paper discusses the advantages of fused silica etalons in hyperfine structure analysis of spectr...
Spectral lines, widths, and shapes are powerful tools for emitting/absorbing gas diagnostics in diff...
We present CLOUDY calculations for the intensity of coronal hyperfine lines in various environments....
Optically excited mercury resonance radiation was used as a light source to provide the sharpest pos...
Spectroscopic methods of measurement of high temperatures are reviewed briefly. They refer mostly to...
We have used H band spectra from IGRINS (R ~45000) of 34 K giants to investigate the limits of infra...
Author Institution: Theoretical Division, T-4 MS B212, Los Alamos National Laboratory; NASA - Goddar...
The hyperfine structure of mercury extracted from neutron irradiated gold has been investigated with...
SUMMARY: Taking into account effects of hyperfine structure, we calculated the synthetic solar spect...
Abstract. We have analysed the 10 m spectral region of a sample of Herbig Ae/Be (HAEBE) stars. The s...
[1] Ch. Salomon, Ch. Breant, Ch. Borde and R.L. Barger J. Physique Colloques 42 C8 (1981) [2] A. Cla...
There are several problems in astrophysics that cannot be addressed until very high resolution spec-...
Hyperfine structure lines of highly-charged ions may open a new window in observations of hot rarefi...
We have applied the technique of speckle masking to spectra. The obser- vation of elongated solar s...
The primary objective of this program was to obtain FUSE observations of the multiple interstellar a...