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,
Saved in:
Author / Creator: | Baxandall, Frank E. |
---|---|
Imprint: | London, Printed for H. M. Stationery off., by Eyre and Spottiswoode, ltd., 1910. |
Description: | vi, 77 p. incl. tables. 31 x 25 cm. |
Language: | English |
Subject: | |
Format: | Print Book |
URL for this record: | http://pi.lib.uchicago.edu/1001/cat/bib/4011511 |
Table of 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.