Elemental abundance analyses with DAO spectrograms - XIX. The superficially normal B stars zeta Draconis, epsilon Lyrae, 8 Cygni and 22 Cygni
Abstract
Elemental abundances of the superficially normal early and middle B stars zeta Dra, epsilon Lyr, 8 Cyg and 22 Cyg are derived, consistent with previous studies in this series, using spectrograms obtained with Reticon and CCD detectors. Almost all of the derived metal abundances are found to be solar within the errors of the analysis. However, the He/H ratios are slightly greater than solar.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 1998
- DOI:
- 10.1046/j.1365-8711.1998.01426.x
- Bibcode:
- 1998MNRAS.296..856A
- Keywords:
-
- STARS: ABUNDANCES;
- STARS: EARLY-TYPE;
- STARS: INDIVIDUAL: ZETA DRACONIS;
- STARS: INDIVIDUAL: EPSILON LYRAE;
- STARS: INDIVIDUAL: 8 CYGNI;
- STARS: INDIVIDUAL: 22 CYGNI