Absorption Line Spectrum of the Quasi-stellar Object 3C 191

Details Absorption Line Spectrum of the Quasi-stellar Object 3C 191 Absorption Line Spectrum of the Quasi-stellar Object 3C 191

Sep 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.215.1045f&link_type=abstract

Nature, Volume 215, Issue 5105, pp. 1045-1046 (1967).

Physics

Scientific paper

BAHCALL1 has pointed out that in the absorption line spectrum for ions in the gaseous envelope of 3C 191, there is a correlation between the ionization potential and Δz, the difference between z (the red-shift of the absorption line spectrum for any ion) and zmacrem (the mean red-shift of the emission line spectrum). Fig. 1 indicates, as a set of vertical lines, the spread in Δz values derived from curves fitted by Burbidge and Lynds2 to four sets of measurements3,4. In the figure, the ionization potential plotted is that of the atom or ion having one more electron than the absorbing ion; while Δz is defined as zmacrem-z.

Affiliated with

Also associated with

No associations

Rating

Absorption Line Spectrum of the Quasi-stellar Object 3C 191 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 Absorption Line Spectrum of the Quasi-stellar Object 3C 191, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Absorption Line Spectrum of the Quasi-stellar Object 3C 191 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1501964