Research Catalog
Researches on the chemical origins of various lines in solar and stellar spectra. Being the results of investigations made at the Solar physics observatory, South Kensington, after discussion
- Title
- Researches on the chemical origins of various lines in solar and stellar spectra. Being the results of investigations made at the Solar physics observatory, South Kensington, after discussion, by Frank E. Baxandall, Solar physics observatory. Under the direction of Sir Norman Lockyer.
- Author
- Baxandall, Frank E.
- Publication
- London, Printed for H. M. Stationery off., by Eyre and Spottiswoode, ltd., 1910.
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Text | Request in advance | OSD+ (Baxandall, F. E. Researches on the chemical origins of various lines in solar and stellar spectra) | Offsite |
Details
- Additional Authors
- Description
- vi, 77 p. incl. tables.; 31 x 25 cm.
- Subject
- Note
- At head of title: Solar physics committee.
- Contents
- I. The spectra of the sun (Fraunhoferic) chromosphere, and lower-type stars in relation to the sun-spot spectrum.--II. The spectrum of E Ursae Majoris.--III. Nitrogen lines in stellar spectra.--IV. Second list of enhanced lines.--V. Lines of simple and definite origin suitable for measurement in radial velocity work on various stellar types.--VI. Lines of unknown origin in various celestial spectra.
- Call Number
- OSD+ (Baxandall, F. E. Researches on the chemical origins of various lines in solar and stellar spectra)
- LCCN
- 11002150
- OCLC
- 11997985
- Author
- Baxandall, Frank E.
- Title
- Researches on the chemical origins of various lines in solar and stellar spectra. Being the results of investigations made at the Solar physics observatory, South Kensington, after discussion, by Frank E. Baxandall, Solar physics observatory. Under the direction of Sir Norman Lockyer.
- Imprint
- London, Printed for H. M. Stationery off., by Eyre and Spottiswoode, ltd., 1910.
- Added Author
- Lockyer, Norman, Sir, 1836-1920.Solar Physics Committee (Great Britain)
- Research Call Number
- OSD+ (Baxandall, F. E. Researches on the chemical origins of various lines in solar and stellar spectra)