The spectrum of the AM star HR 178 - Line identifications and equivalent widths in the range 3800 to 6700 A

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

7

A Stars, Abundance, Giant Stars, Hertzsprung-Russell Diagram, Peculiar Stars, Spectral Line Width, Stellar Spectra, Astronomical Catalogs, Spectrum Analysis

Scientific paper

The present 3800-6700 A line identifications and equivalent widths for the Am star HR 178 were produced by a reduction procedure that used a Fourier transform analysis to suppress high frequencies that are due to photographic emulsion noise. In order to eliminate systematic instrumental effects between these spectra and those of 15 Vul, spectra are also obtained for this star using the same methods. It is found that the best agreements exist among the different abundance determinations for each element from neutral and ionized stages, in both absolute and differential growth curves, for the blue and red spectral ranges.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The spectrum of the AM star HR 178 - Line identifications and equivalent widths in the range 3800 to 6700 A 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 spectrum of the AM star HR 178 - Line identifications and equivalent widths in the range 3800 to 6700 A, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectrum of the AM star HR 178 - Line identifications and equivalent widths in the range 3800 to 6700 A will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1829579

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.