Emission features in moderate-redshift QSO spectra shortward of Lyman alpha

Details Emission features in moderate-redshift QSO spectra shortward of Lyman alpha Emission features in moderate-redshift QSO spectra shortward of Lyman alpha

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.269s&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 269-272 (SEE N89

Astronomy and Astrophysics

Astronomy

2

Iue, Lyman Beta Radiation, Quasars, Spaceborne Astronomy, Ultraviolet Astronomy, Ultraviolet Spectra, Emission Spectra, Line Spectra, Lyman Spectra, Red Shift

Scientific paper

Thirty-nine IUE images were used to study emission features shortward of H I Lyman alpha in quasars. The images represent 22 moderate-redshift (0.35 less than or equal to Z less than or equal to 0.66) quasars. The features due to S VI, C III, N III, O VI - Ly Beta, S IV, and N II are quite common for the quasars of the data sample. Below the Lyman limit at 912A, features become much more difficult to identify. Emission features arising from C II (902A) and O II to O III (934A) each in one spectrum, are tentatively identified.

Affiliated with

Also associated with

No associations

Rating

Emission features in moderate-redshift QSO spectra shortward of Lyman alpha 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 Emission features in moderate-redshift QSO spectra shortward of Lyman alpha, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emission features in moderate-redshift QSO spectra shortward of Lyman alpha will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1180940