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Models of very-low-mass stars, brown dwarfs and exoplanets
Within the next few years, GAIA and several instruments aiming to image extrasolar planets will be ready. In parallel, low-mass planets are being sought around red dwarfs, which offer more favourable conditions, for both radial velocity detection and transit studies, than solar-type stars. In this p...
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| Main Authors: | , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
The Royal Society Publishing
2012
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| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3350648/ https://ncbi.nlm.nih.gov/pubmed/22547243 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2011.0269 |
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