|
|
Paper: |
PHOENIX Spectra of Red Supergiants—Varying the Surface Abundances and the Microturbulence |
Volume: |
425, Hot and Cool: Bridging Gaps in Massive Star Evolution |
Page: |
61 |
Authors: |
Lançon, A.; Hauschildt, P. H. |
Abstract: |
Based on PHOENIX models, we briefly discuss effects of surface abundances and microturbulence on the near-IR spectra of red supergiant stars. |
|
|
|
|