The abundances of the elements in sharp-lined early type stars

Details The abundances of the elements in sharp-lined early type stars The abundances of the elements in sharp-lined early type stars

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cccscrept.....a&link_type=abstract

Final Report, 1 May - 31 Jul. 1992 Citadel Coll., Charleston, SC. Dept. of Physics.

Physics

A Stars, Abundance, B Stars, Iue, Main Sequence Stars, Stellar Composition, Line Spectra, Metallic Stars, Ultraviolet Spectra

Scientific paper

An International Ultraviolet Explorer (IUE) observing strategy that has yielded co-added spectra with enhanced S/N ratios for several A and B stars was established. New observations by Roby and Adelman using the same technique were added two new Hg-Mn stars into this sample. A long-term study of elemental abundances in this uniform, high-quality set of IUE spectra for 13 stars was begun. The first stages of this project are reported: abundances for N, Cr, Mn, Fe, Co, and Ni. The study of the Fe-peak elements show that our data set can provide accurate abundances and that abundances obtained from UV and optical spectra often are in good agreement. The groundwork for selfconsistent abundance analyses of more exotic elements in our long term project was provided.

Affiliated with

Also associated with

No associations

Rating

The abundances of the elements in sharp-lined early type stars 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 abundances of the elements in sharp-lined early type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The abundances of the elements in sharp-lined early type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1166547