Fingerprint
Dive into the research topics of 'Non-LTE abundance corrections for late-type stars from 2000Å to 3μm I. Na, Mg, and Al'. Together they form a unique fingerprint.- Sort by
- Weight
- Alphabetically
Non-LTE abundance corrections for late-type stars from 2000Å to 3μm I. Na, Mg, and Al
K. Lind, T. Nordlander, A. Wehrhahn, M. Montelius, Y. Osorio, P. S. Barklem, M. Afsar, C. Sneden, C. Kobayashi
Research output: Contribution to journal › Article › peer-review
10
Downloads
(Pure)