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Bands of NaH lines in Spectra of Late Type Stars
Yu P. Lyubchyk
, Ya V. Pavlenko
, O. K. Lyubchyk
,
H. R.A. Jones
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Centre for Astrophysics Research (CAR)
Research output
:
Contribution to journal
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Article
›
peer-review
2
Citations (Scopus)
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Keyphrases
Dissociation
100%
MSTAR
100%
Late-type Stars
100%
Stellar Atmospheres
100%
Synthetic Spectra
100%
Teff
50%
Red Dwarfs
50%
Spectral Energy Distribution
50%
Strong Absorption
50%
Complicated Task
50%
Temperature Rise
50%
Model Atmospheres
50%
Near-infrared
50%
Chemical Composition
50%
Opacity
50%
Line Detection
50%
Solar Fuels
50%
Visible-infrared
50%
Effective Temperature
50%
ExoMol
50%
Sodium Hydride
50%
Energy Distribution
50%
Atmospheric Parameters
50%
Parameter Calculation
50%
Radiation Absorption
50%
Physics
Stellar Atmosphere
100%
M Stars
100%
Late-Type Stars
100%
M Giant Stars
50%
Spectral Energy Distribution
50%
Energy Distribution
50%
Near Infrared
50%