Vibration-rotational intensities for the X 1Sigma(+) state of A1H and A1D

Details Vibration-rotational intensities for the X 1Sigma(+) state of A1H and A1D Vibration-rotational intensities for the X 1Sigma(+) state of A1H and A1D

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...323..810t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 323, Dec. 15, 1987, p. 810-813. Research supported by the U.S.-Spanish Comm

Mathematics

Logic

4

Diatomic Molecules, Ground State, Quantum Mechanics, Rotating Plasmas, Stellar Atmospheres, Vibrational Spectra, Cool Stars, Dipole Moments, Least Squares Method, Schroedinger Equation

Scientific paper

Vibration-rotational line strengths (Einstein A-coefficients) for the ground electronic state (X 1Σ+) of AlH and AlD have been calculated for the following sets of vibrational and rotational quantum numbers: 0 ≤ Δυ ≤ 5 for 0 ≤ υarcmin ≤ 15, and Jarcmin - J = ±1 for 0 ≤ Jarcmin ≤ 50. Representative numerical results are presented, and the possibility of observing these transitions in stellar spectra is briefly discussed.

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