Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263..409b&link_type=abstract
In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 409-41
Astronomy and Astrophysics
Astrophysics
1
Line Spectra, Peculiar Stars, Stellar Composition, Stellar Spectra, Ultraviolet Spectra, Abundance, Cobalt, Iron, Iue, Radial Velocity
Scientific paper
Element identifications in the long wavelength IUE spectrum of HD 101065 (Przybylski's star) made using the method of wavelength coincidence statistics are reported. The definite presence of the common iron-peak elements, in addition to numerous doubly ionized rare-earth species, is confirmed. Radial velocity sweeps yield no strong evidence of segregation between the iron-peak and lanthanide rare-earth elements in this star. New evidence to support the identification of Co I and Co II is also presented. The similarity between HD 101065 and several hot, magnetic Ap stars which also exhibit an unusually strong presence of cobalt relative to iron is noted.
Bord Donald J.
Desko R. D.
No associations
LandOfFree
An analysis of the ultraviolet spectrum of HD 101065 by line coincidence statistics 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 An analysis of the ultraviolet spectrum of HD 101065 by line coincidence statistics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An analysis of the ultraviolet spectrum of HD 101065 by line coincidence statistics will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1294870