The /Mg-24/H molecule in the atmospheres of late type stars - Transition probabilities, oscillator strengths, and fine structures of rotation-vibration bands

Details The /Mg-24/H molecule in the atmospheres of late type stars - Transition probabilities, oscillator strengths, and fine structures of rotation-vibration bands The /Mg-24/H molecule in the atmospheres of late type stars - Transition probabilities, oscillator strengths, and fine structures of rotation-vibration bands

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....54..417m&link_type=abstract

Astronomy and Astrophysics, vol. 54, no. 2, Jan. 1977, p. 417-424.

Astronomy and Astrophysics

Astrophysics

5

Late Stars, Magnesium Compounds, Metal Hydrides, Molecular Spectra, Stellar Atmospheres, Transition Probabilities, Abundance, Atmospheric Composition, Fine Structure, Molecular Oscillations, Molecular Rotation, Stellar Spectra

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1977A&A....54..417M

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