On the atmosphere of the star HD 103877.
Abstract
A study of the spectrum of HD 103877 suggests that it is an evolved early F type star with apparent surface abundance anomalies typical of the classical Am stars. This agrees with the predictions of the element separation mechanism and recent model envelope calculations.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- 1972
- DOI:
- 10.1093/mnras/159.1.29P
- Bibcode:
- 1972MNRAS.159P..29S