Sobre la correlación entre exceso de color y luminosidad
It is found that is unnecessary to deal with circumstellar shells to explain the apparent correlation between reddening and luminosity in young stellar groups. The simple combination of the luminosity function and a color excess distribution can reproduce the observed appearance of the luminosity vs...
Guardado en:
| Autor principal: | |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1980
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/99238 |
| Aporte de: |
| Sumario: | It is found that is unnecessary to deal with circumstellar shells to explain the apparent correlation between reddening and luminosity in young stellar groups. The simple combination of the luminosity function and a color excess distribution can reproduce the observed appearance of the luminosity vs. color excess diagram of Cygnus II including the lack of little reddened high luminosity stars. |
|---|