An analysis of vibration-rotation lines of OH in the solar infrared spectrum

Grevesse, N.; Sauval, A.J.; Dishoeck, E.F. van (1984)

Article / Letter to editor

High resolution solar spectra have permitted the measurement with great accuracy of equivalent widths of vibration-rotation lines of OH in the X2Pi state near 3-micron wavelength. Using recent theoretical results for the transition probabilities, a solar oxygen abundance of (8.93 + or - 0.02) is derived which is in perfect agreement with the abundance deduced from the OH pure rotation lines. The solar abundance of oxygen is therefore A(O) = 8.92 + or - 0.035, as inferred from the analysis of 43 vibration-rotation lines and 81 pure rotation lines of the OH molecule. It is confirmed that the dipole moment function of Werner, Rosmus and Reinsch (1983) together with the Holweger-Mueller (1974) solar atmosphere model are to be preferred in the analysis of the data.

• abundance
• hydroxyl emission
• oscillator strengths
• solar spectra
• stellar composition
• vibrational spectra
• dipole moments
• infrared spectra
• oxygen
• solar atmosphere
• spectral line width
• transition probabilities

• All authors: Grevesse, N.; Sauval, A.J.; Dishoeck, E.F. van
• Date: 1984