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...
Salvato in:
| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autori principali: | , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2008
|
| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57144115 |
| Tags: |
Nessun Tag, puoi essere il primo ad aggiungerne!!
|