Optical region elemental abundance analyses of B and A stars. I - PI Ceti, 134 Tauri, HR 2154, HR 5780, 21 Aquilae and NU Capricorni

Details Optical region elemental abundance analyses of B and A stars. I - PI Ceti, 134 Tauri, HR 2154, HR 5780, 21 Aquilae and NU Capricorni Optical region elemental abundance analyses of B and A stars. I - PI Ceti, 134 Tauri, HR 2154, HR 5780, 21 Aquilae and NU Capricorni

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.206..637a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 206, Feb. 1, 1984, p. 637-648. Research supported by th

Astronomy and Astrophysics

Astronomy

38

A Stars, Abundance, B Stars, Spectrum Analysis, Stellar Atmospheres, Visible Spectrum, H Beta Line, Late Stars, Main Sequence Stars, Solar Atmosphere, Spectral Energy Distribution, Stellar Models

Scientific paper

Abundance analyses using optical region data and fully line blanketed
model atmospheres have been performed for six moderately sharp-lined
middle to late B-type stars. The derived abundances have values similar
to those of the Sun.

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