Observed Energy Distribution of α Lyra and β Cen at 2000-3800 Å

Details Observed Energy Distribution of α Lyra and β Cen at 2000-3800 Å Observed Energy Distribution of α Lyra and β Cen at 2000-3800 Å

Sep 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.239...90g&link_type=abstract

Nature, Volume 239, Issue 5367, pp. 90 (1972).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

THE space astrophysical observatory Orion, installed in the orbital station Salyut, has provided several slitless spectrograms of α Lyra and β Cen between wavelengths 2000 and 3800 Å. The spectrograms were obtained in June 1971 with the help of a mirror telescope of the Mersenn system and a spectrograph of the Wadsworth system using film sensitive in the far ultraviolet. The dispersion of the spectrograph is 32 Å/mm, while the resolution of the spectrograms derived is about 5 Å on 2600 Å. A detailed description of the Orion apparatus and the method of obtaining the spectrograms have been given elsewhere1-3.

Affiliated with

Also associated with

No associations

Rating

Observed Energy Distribution of α Lyra and β Cen at 2000-3800 Å does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Observed Energy Distribution of α Lyra and β Cen at 2000-3800 Å, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observed Energy Distribution of α Lyra and β Cen at 2000-3800 Å will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-987831