Last edited by Shabei
Sunday, April 19, 2020 | History

2 edition of Application of the DDO reticon system to G and K star abundance studies and Nova Cygni 1975 found in the catalog.

Application of the DDO reticon system to G and K star abundance studies and Nova Cygni 1975

Bruce Thomas Evison Campbell

Application of the DDO reticon system to G and K star abundance studies and Nova Cygni 1975

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  • 12 Currently reading

Published by s.n.] in [Toronto .
Written in English

    Subjects:
  • Astronomical spectroscopy,
  • G stars,
  • O stars,
  • Stars, New

  • Edition Notes

    StatementBruce Campbell.
    ContributionsToronto, Ont. University.
    The Physical Object
    Paginationiv, 62 p. :
    Number of Pages62
    ID Numbers
    Open LibraryOL19064772M


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Application of the DDO reticon system to G and K star abundance studies and Nova Cygni 1975 by Bruce Thomas Evison Campbell Download PDF EPUB FB2

Spectroscopic study of the star Canum Venat (G0). NASA Astrophysics Data System (ADS) Mentese, H. In this work the effective temperature and surface gravity of the star BetaCVn were determined by means of the theoretical profiles calculated by De Jager and Neven (). The best agreement was obtained for T(eff) = K and log g = 4.

Abundance Analysis of the Helium Weak Star TAURI. NASA Astrophysics Data System (ADS) Mon, M.; Hirata, R.; Sadakane, K. An abundance analysis of the helium-weak star 20 Tauri is performed with a fully line-blanketed model atmosphere. The adopted atmospheric parameters are Teff = K and log g.

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NASA Images Solar System Collection Ames Research Center. Brooklyn Museum. Full text of "Year book - Carnegie Institution of Washington" See other formats.