Abstract
We present an analysis of a high-resolution (R ≅ 40 000) infrared spectrum of the RS Oph secondary around the first overtone CO bands, obtained in 2008 May on the Gemini-South 8 m telescope. The 12CO and 13CO bands are well resolved, and we compute synthetic spectra to determine the 12C/13C ratio. We find 12C/13C ≅ 16 ± 3, consistent with the interpretation of the secondary as a red giant which has evolved beyond the first dredge-up phase of evolution.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 206-211 |
| Number of pages | 6 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 404 |
| Issue number | 1 |
| DOIs | |
| State | Published - May 2010 |
Keywords
- Binaries: Symbiotic
- Cataclysmic variables
- Novae
- Stars: Abundances
- Stars: Individual: RS Oph