Direct detection of exo-planets: GQ Lupi

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dc.creatorNeuhaeuser, Ralph
dc.creatorGuenther, Eike
dc.creatorHauschildt, Peter
dc.date2005-06-01
dc.date.accessioned2026-07-07T02:17:53Z
dc.date.available2026-07-07T02:17:53Z
dc.descriptionWe 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.
dc.descriptionProceedings ESO Workshop on The power of optical/IR interferometry
dc.identifierhttps://arxiv.org/abs/astro-ph/0506011
dc.identifierhttp://arxiv.org/abs/astro-ph/0506011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9283
dc.subjectAstrophysics
dc.titleDirect detection of exo-planets: GQ Lupi
dc.typetext

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