arXiv · 0905.0439
Homogeneous comparison of planet candidates imaged directly until 2008
Abstract
We present a compilation of the planet candidates currently known from direct imaging. We have gathered available data from the literature and derive the luminosity of all candidates in a homogeneous way using a bolometric correction, the distances and the K band magnitudes of the objects. In a final step we find the masses of the candidates from a comparison of the luminosity or, if not available, an absolute brightness and several well known hot-start evolutionary models.
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T. O. B. Schmidt, R. Neuhäuser, A. Seifahrt. 2009-05-12. Homogeneous comparison of planet candidates imaged directly until 2008. https://doi.org/10.1063/1.3215849
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