Doppler Tomography of Cataclysmic Variables with a 6.5-m class Telescope
We are conducting a long-term project of high dispersion spectroscopy (R 20000) to observe and analyzea sample of cataclysmic variables with the 2.1-m telescope at San Pedro Mártir and the echelle spectrograph.The main tool for this analysis is Doppler tomography. In this contribution we summarize o...
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2007 |
| País: | México |
| Recursos: | Universidad Nacional Autónoma de México |
| Repositorio: | Redalyc-UNAM |
| OAI Identifier: | oai:redalyc.org:57102825 |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57102825 |
| Access Level: | acceso abierto |
| Palavra-chave: | Física, Astronomía y Matemáticas TECH TELESCOPES NIQUES: SPECTROSCOPIC TECHNIQUES: MISCELLANEOUS NOVAE: CATACLYSMIC VARIABLES |
| Resumo: | We are conducting a long-term project of high dispersion spectroscopy (R 20000) to observe and analyzea sample of cataclysmic variables with the 2.1-m telescope at San Pedro Mártir and the echelle spectrograph.The main tool for this analysis is Doppler tomography. In this contribution we summarize our work and posethe question: how can we improve this project with a 6.5-m class telescope? |
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