Últimos resultados en el análisis evolutivo del cumulo abierto NGC 2527
Abstract:We present a spectroscopic analysis of 13 (V < 11) stars in the open cluster NGC 2527. We carried out a study of radial velocity variability and kinematic membership of the observed stars. One of members is a blue straggler, for which we discuss possible formation scenarios. Furthermore,...
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| Autores principales: | , , |
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| Formato: | conferenceObject |
| Lenguaje: | Español |
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Asociación Argentina de Astronomía
2021
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| Materias: | |
| Acceso en línea: | http://hdl.handle.net/11086/18944 |
| Aporte de: |
| Sumario: | Abstract:We present a spectroscopic analysis of 13 (V < 11) stars in the open cluster NGC 2527. We carried out a study of radial velocity variability and kinematic membership of the observed stars. One of members is a blue straggler, for which we discuss possible formation scenarios. Furthermore, using the SPM4 catalog we perform a star count in order to determine the Initial Mass Function and to estimate the stellar mass loss in the cluster. |
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