Una nueva interpretación de los recuentos estelares promedios de Seares, van Rhijn, Joyner y Richmond 1925 Ap.J. 62
These stellar recounts averaged over all galactic latitudes are analysed by a series of Kapteyn-schemes. In this way, “artificial” stellar count without and with general interstellar absorption are originated. All these curves can be represented, almost until m=20, by one unique interpolation formul...
Guardado en:
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1971
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/98560 |
| Aporte de: |
| Sumario: | These stellar recounts averaged over all galactic latitudes are analysed by a series of Kapteyn-schemes. In this way, “artificial” stellar count without and with general interstellar absorption are originated. All these curves can be represented, almost until m=20, by one unique interpolation formula, function of the galactic latitude and of the apparent magnitude. |
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