Spectral energy distribution for GJ406

We present results of modelling the bulk of the spectral energy distribution (0.35–5 μm) for GJ406 (M6V). Synthetic spectra were calculated using the NextGen, Dusty and Cond model atmospheres and incorporate line lists for H2O, TiO, CrH, FeH, CO, MgH molecules as well as the VALD line list of atomic...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2006-02, Vol.447 (2), p.709-717
Hauptverfasser:	Pavlenko, Ya. V., Jones, H. R. A., Lyubchik, Yu, Tennyson, J., Pinfield, D. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology molecular data stars: atmospheres stars: evolution stars: fundamental parameters stars: individual: GJ406 stars: late-type
Online-Zugang:	Volltext
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