Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-09T19:46:58.909Z Has data issue: false hasContentIssue false
  • English
  • Français

15. Detection of the spectral line of deuterium from the centre of the Galaxy on the wave-length of 91·6 cm.

Published online by Cambridge University Press:  14 August 2015

G. G. Getmanzev ,
K. S. Stankevitch  and
V. S. Troitzky
G. G. Getmanzev
Affiliation:
Gorky State University, U.S.S.R.
K. S. Stankevitch
Affiliation:
Gorky State University, U.S.S.R.
V. S. Troitzky
Affiliation:
Gorky State University, U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

As was shown by I. S. Shklovsky, a radio spectral line from interstellar deuterium on λD = 91·6 cm. (fD = 327·38424 Mc./s.) may be expected [1]. According to Shklovsky the difference between the effective temperature Teff in this line and outside it must be of the order of 1/500 Teff in the direction of the galactic centre, if the concentration of deuterium equals 10−3 that of hydrogen. In this case, contrary to the emission by hydrogen, an absorption line is expected. As Teff equals about 300° the depth should be of the order of 0·6°.

Type
Part I: Spectral Line Investigations
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 90 - 91
Copyright
Copyright © Cambridge University Press 1957 

References

1. Shklovsky, I. S. A.J. U.S.S.R. 29, 144, 1952.Google Scholar