Ultraviolet Stellar Spectroscopy on Gemini 11

Details Ultraviolet Stellar Spectroscopy on Gemini 11 Ultraviolet Stellar Spectroscopy on Gemini 11

Mar 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967sci...155.1407h&link_type=abstract

Science, Volume 155, Issue 3768, pp. 1407-1408

Physics

10

Scientific paper

Objective-prism and objective-grating spectrograms were obtained in six star fields during the Gemini 11 mission. The grating spectra show absorption lines in the 2000 to 3000 angstrom wavelength region of Canopus and Sirius and provide ultraviolet-energy distribution data for approximately 50 stars. Many prism spectra show the Balmer discontinuity due to hydrogen and two absorption features probably due to ultraviolet iron multiplets.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet Stellar Spectroscopy on Gemini 11 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 Ultraviolet Stellar Spectroscopy on Gemini 11, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet Stellar Spectroscopy on Gemini 11 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1313520