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Cited article:
B. Fuhrmeister, C. I. Short, P. H. Hauschildt
A&A, 452 3 (2006) 1083-1088
Published online: 2006-06-06
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SEMIEMPIRICAL MODELS OF THE SOLAR ATMOSPHERE. III. SET OF NON-LTE MODELS FOR FAR-ULTRAVIOLET/EXTREME-ULTRAVIOLET IRRADIANCE COMPUTATION
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The effects of new $\ion{Na}{i}$ D line profiles in cool atmospheres
C. M. S. Johnas, P. H. Hauschildt, A. Schweitzer, et al.
Astronomy & Astrophysics 466 (1) 323 (2007)
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The effects of new Na I D line profiles in cool atmospheres
C. M. S. Johnas, P. H. Hauschildt, A. Schweitzer, et al.
Astronomy & Astrophysics 475 (3) 1039 (2007)
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The influence of dust formation modelling on Na i and K i line profiles in substellar atmospheres
C. M. S. Johnas, Ch. Helling, M. Dehn, P. Woitke and P. H. Hauschildt
Monthly Notices of the Royal Astronomical Society: Letters 385 (1) L120 (2008)
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Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets around Low-mass Stars: The TRAPPIST-1 System
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Multi-wavelength observations of a giant flare on CN Leonis
B. Fuhrmeister, J. H. M. M. Schmitt and P. H. Hauschildt
Astronomy and Astrophysics 511 A83 (2010)
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The CARMENES search for exoplanets around M dwarfs
D. Hintz, B. Fuhrmeister, S. Czesla, et al.
Astronomy & Astrophysics 623 A136 (2019)
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