Measurement of relative intensities of Fe I lines of astrophysical interest

Details Measurement of relative intensities of Fe I lines of astrophysical interest Measurement of relative intensities of Fe I lines of astrophysical interest

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jqsrt..41..433m&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 41, June 1989, p. 433-438.

Astronomy and Astrophysics

Astrophysics

5

Astrophysics, Emission Spectra, Iron, Numerical Control, Spectral Line Width, Microcomputers, Spectrometers

Scientific paper

The intensities of selected Fe I lines of astrophysical interest were measured relative to the intensity of stronger lines having a common upper energy level. The error in the measured intensity ratios is estimated to be 7 percent. The measured intensity ratios were converted into absolute f-values for the weak lines using known f-values for the reference line.

Affiliated with

Also associated with

No associations

Rating

Measurement of relative intensities of Fe I lines of astrophysical interest 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 Measurement of relative intensities of Fe I lines of astrophysical interest, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurement of relative intensities of Fe I lines of astrophysical interest will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1855784