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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Details

Additional Authors
  • Lockyer, Norman, Sir, 1836-1920.
  • Solar Physics Committee (Great Britain)
Description
vi, 77 p. incl. tables.; 31 x 25 cm.
Subject
  • Spectrum, Solar
  • Stars > Spectra
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)
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