Chemical composition in fast rotators main sequence stars
Using public data of the Ultraviolet and Visual Echelle Spectrograph ParanalObservatory Project (UVES POP) the projected rotational velocities, v sin i, for 16stars in the field of the galactic cluster IC 2391 (o Vel Cluster) were obtained usingthe method of the Fourier transform (FT). We found that...
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| I publikationen: | Revista Mexicana de Astronomía y Astrofísica |
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| Huvudupphov: | , |
| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
Universidad Nacional Autónoma de México
2008
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| Ämnen: | |
| Länkar: | https://www.redalyc.org/articulo.oa?id=57144115 |
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