WFRF:(Leckrone DS)
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- Wahlgren, GlennLund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science (author)
Very heavy elements in the HgMn star chi Lupi
- Article/chapterEnglish1998
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- 1998
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- LIBRIS-ID:oai:lup.lub.lu.se:ccac68b8-d78a-44be-b851-870874c45ee3
- https://lup.lub.lu.se/record/3919550URI
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- Language:English
- Summary in:English
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- Abundances for the elements W, Os, and Bi are presented for the HgMn star chi Lupi, based upon GHRS echelle-mode spectra and a synthetic spectrum analysis. The tungsten abundance is consistent with a solar-system value while the osmium and bismuth abundances reflect enhancements. With these new data we are able to quantitatively define an abundance peak within the element range Z = 74 through 83.
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- Leckrone, DS (author)
- Brage, TomasLund University,Lunds universitet,Naturvetenskapliga fakulteten,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Faculty of Science,Department of Physics,Departments at LTH,Faculty of Engineering, LTH(Swepub:lu)nucl-tbr (author)
- Proffitt, CR (author)
- Johansson, SvenericLund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science(Swepub:lu)fysi-sjo (author)
- Astronomi - Genomgår omorganisationInstitutionen för astronomi och teoretisk fysik - Genomgår omorganisation (creator_code:org_t)
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- In:The Scientific Impact of the Goddard High Resolution Spectrograph (Astronomical Society of the Pacific Conference Series)143, s. 330-3331886733635
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