A comment on the spectral energy distributions of Ba II stars.
Abstract
Contrary to a recent suggestion, the 4000 A flux depressions of the Ba ii stars are shown not to be caused by increased strengths of CN, CH and C2 bands but rather by a wide, apparently continuous, spectral feature.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- December 1975
- DOI:
- 10.1093/mnras/173.1.83P
- Bibcode:
- 1975MNRAS.173P..83F