Direct detection of exo-planets: GQ Lupi

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We present a comparison of our VLT/NACO K-band spectrum of the GQ Lupi companion with the new GAIA-dusty model atmosphere grid for T=2000 and 2900 K and log g from 0 to 4. Then, we discuss the mass estimate for GQ Lup companion.
Proceedings ESO Workshop on The power of optical/IR interferometry

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/9283

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0506011
 http://arxiv.org/abs/astro-ph/0506011

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arXiv