Hβ photometry for UVBY standard stars
From 1984 to 1986 the authors made several observational campaigns at Calar Alto and La Palma Observatories using the uvby and β photometric systems to monitor a selected sample of late-type variable stars. In this paper they present the β values for 38 uvby standard stars to contribute to the uvby-...
| Autores: | , , , , , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 1988 |
| País: | España |
| Institución: | Universidad Complutense de Madrid (UCM) |
| Repositorio: | Docta Complutense |
| Idioma: | inglés |
| OAI Identifier: | oai:docta.ucm.es:20.500.14352/57957 |
| Acceso en línea: | https://hdl.handle.net/20.500.14352/57957 |
| Access Level: | acceso abierto |
| Palabra clave: | 52 Late stars Stellar luminosity Stellar spectrophotometry Ubv spectra Variable stars Calibrating Cassegrain optics Linear equations Astronomy Photometry Astrofísica Astronomía (Física) |
| Sumario: | From 1984 to 1986 the authors made several observational campaigns at Calar Alto and La Palma Observatories using the uvby and β photometric systems to monitor a selected sample of late-type variable stars. In this paper they present the β values for 38 uvby standard stars to contribute to the uvby-β calibration works on late-type stars. In the final discussion, the β computed values are plotted against the Stroemgren b-y, m_(1), and c_(1) indices. |
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