Ca II H and K reversals in carbon stars.
Abstract
Nine heavily exposed, high-dispersion blue spectrograms of seven different hot carbon stars were obtained. All spectra show a reversal in the Ca ii H and K lines. The widths of the reversals were measured and, after establishing a calibration, the absolute visual magnitudes of the seven stars were derived. Four of the stars, all ordinary R stars, have absolute magnitudes and colors which place them close to the normal giant branch in the spectral range 08 to K2. The remaining three stars are all hydrogen-deficient carbon stars. All these stars are supergiants, lying along the Ib supergiant branch in a color-magnitude diagram. Subject headings: Ca ii emission - carbon stars - hydrogen-deficient stars - luminosities
- Publication:
-
The Astrophysical Journal
- Pub Date:
- May 1975
- DOI:
- 10.1086/153550
- Bibcode:
- 1975ApJ...197..611R