The identification of high-level transitions of Fe II in stellar spectra

Details The identification of high-level transitions of Fe II in stellar spectra The identification of high-level transitions of Fe II in stellar spectra

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...139..243j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 139, no. 1, Oct. 1984, p. 243-247.

Astronomy and Astrophysics

Astrophysics

11

Peculiar Stars, Stellar Atmospheres, Stellar Spectra, A Stars, B Stars, Iron, Line Spectra

Scientific paper

Positive identifications are made in four B and A-type stellar spectra of lines from 3d6(5D)4d-3d6(5D)4f transitions in Fe II. The lowest levels of the 4d terms have excitation energies of 10.3 eV, while those of the 4f terms are at 12.8 eV. Numerous features that were previously unidentified in B and A stars may now be explained. The obvious presence of such transitions makes it probable that many other high-level transitions are present in stellar spectra. Some of these transitions have not yet been identified in laboratory studies analyses, but they could be of considerable importance in the chemical analyses of stellar atmospheres.

Affiliated with

Also associated with

No associations

Rating

The identification of high-level transitions of Fe II in stellar spectra 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 The identification of high-level transitions of Fe II in stellar spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The identification of high-level transitions of Fe II in stellar spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1226368