Is a new site for the i-process really needed?
Abstract
We present our recent paper Karinkuzhi et al. 2021, A&A, 645, 61 titled: "Low-mass, low-metallicity stars as an efficient i-process site explaining CEMP-rs stars" as a poster.
- Publication:
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The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (CS20.5)
- Pub Date:
- March 2021
- DOI:
- 10.5281/zenodo.4564212
- Bibcode:
- 2021csss.confE.140K
- Keywords:
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- Post main-sequence cool stars