The abundances of Pt, Au, and HG in the chemically peculiar HgMn-type stars kappa CANCRI and chi LUPI
Författare
Summary, in English
Echelle mode spectra obtained with the Goddard High Resolution Spectrograph onboard the Hubble Space Telescope have been used to determine the abundances of the heavy elements Pt, Au, and Hg in the chemically peculiar HgMn-type stars kappa Cancri and chi Lupi. The abundances were determined by fitting observed line profiles with synthetically generated spectra and are found to be enhanced relative to solar system values by between three and five orders of magnitude in both stars. The Hg isotope mixture in kappa Cancri is found to resemble the terrestrial mixture while that of chi Lupi is dominated by the heaviest isotope. As determined from multiple ionization states, the abundances place constraints upon theories attempting to explain the large surficial abundances of heavy elements.
Publiceringsår
1995
Språk
Engelska
Sidor
438-451
Publikation/Tidskrift/Serie
Astrophysical Journal
Volym
444
Issue
1
Dokumenttyp
Artikel i tidskrift
Förlag
American Astronomical Society
Ämne
- Astronomy, Astrophysics and Cosmology
Nyckelord
- CANCRI
- INDIVIDUAL (KAPPA
- ABUNDANCES
- CHEMICALLY PECULIAR
- STARS
- CHI LUPI)
- ULTRAVIOLET
- SPECTRA
Status
Published
ISBN/ISSN/Övrigt
- ISSN: 0004-637X