Optical region elemental abundance analyses of B and A stars - I. PI Ceti, 134 Tauri, HR 2154, HR 5780, 21 Aquilae and NU Capricorni
Open Access
- 1 February 1984
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 206 (3) , 637-648
- https://doi.org/10.1093/mnras/206.3.637
Abstract
Abundance analyses using optical region data and fully line blanketed model atmospheres have been performed for six moderately sharplined middle to late B-type stars. The derived abundances have values similar to those of the Sun.Keywords
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