The Riddle of the Gaseous Nebulae
@article{Hirsh1979TheRO, title={The Riddle of the Gaseous Nebulae}, author={R. Hirsh}, journal={Isis}, year={1979}, volume={70}, pages={197 - 212} }
spectrum that he was accustomed to seeing from stellar bodies, Huggins observed an intense green line and a few fainter ones-indications of the body's gaseous nature. In trying to discover which terrestrial gases emitted these lines, Huggins and his contemporaries utilized two standard techniques in experimental spectroscopy, but without achieving success. A theoretical approach associated with an ad hoc speculation early in the second decade of the twentieth century fared as poorly. Only with… CONTINUE READING
7 Citations
The Cosmos in Your Pocket: How Cosmological Science Became Earth Technology. I
- Philosophy, Physics
- 2007
- PDF
References
SHOWING 1-10 OF 13 REFERENCES
The results of these calculations are
- The Theory of Atomic Spectra
- 1934
" The Intensities of Certain Nebular Lines and the Mean Lives Emitting Them
- Proc . Roy . Soc .
- 1932
For other applications of Bowen ' s interpretation of metastability see P . W . Merrill , " Identification of Lines in the Spectrum of - q Carinae
- Monthly Notices
- 1927
For other applications of Bowen's interpretation of metastability see P
- The Origin of the Nebular Lines and the Structure of the Planetary Nebulae
- 1927
Having solved the nebular riddle, Bowen then unsuccessfully tried to identify some spectral lines in the solar corona that had been attributed to the hypothetical element "coronium
- Wavelengths of Forbidden Nebular Lines
- 1927