The paschen discontinuity in B stars
Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep.
| Autor: | |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 1969 |
| País: | Argentina |
| Institución: | Universidad Nacional de La Plata |
| Repositorio: | SEDICI (UNLP) |
| Idioma: | inglés |
| OAI Identifier: | oai:sedici.unlp.edu.ar:10915/131085 |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/131085 |
| Access Level: | acceso abierto |
| Palabra clave: | Astronomía Ciencias Astronómicas Paschen discontinuity Balmer discontinuity |
| Sumario: | Measurements of the Paschen discontinuity in stars withT eff ≥104K leads to the conclusion that the D P/DB ratio increases with temperature faster than expected. The increase of D P/DB with (logg)−1 is also steep. |
|---|