OGLE-2005-BLG-153: Microlensing Discovery and Characterization of a Very Low Mass Binary
The mass function and statistics of binaries provide important diagnostics of the star formation process. Despite this importance, the mass function at low masses remains poorly known due to observational difficulties caused by the faintness of the object
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2010 |
| País: | Chile |
| Idioma: | inglés |
| OAI Identifier: | oai:repositorio.anid.cl:10533/240748 |
| Acceso en línea: | https://hdl.handle.net/10533/240748 |
| Access Level: | acceso abierto |
| Sumario: | The mass function and statistics of binaries provide important diagnostics of the star formation process. Despite this importance, the mass function at low masses remains poorly known due to observational difficulties caused by the faintness of the object |
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