Abstract
The Zeeman effect on lines in the (0,0) band of the B 3Π-X3 Δ (γ′) system and in the (0,0) band of the A 3Φ-X3 Δ (γ) system of titanium monoxide, TiO, have been recorded and analyzed. Magnetic tuning of the low rotational spectral features recorded at high resolution (FWHM ≃ 35 MHz) and at field strengths of up to 1.2 kG is accurately modeled using an effective Zeeman Hamiltonian. A comparison is made with previous predictions, which were based on field-free spectroscopic parameters. It is shown that the large Λ-doubling in the B 3Π state necessitates the inclusion of ΔJ = ±1 matrix elements in the representation of the effective Hamiltonian operator. The observed spectra could only be modeled by allowing the electronic spin and orbital magnetic g-factors, gs and gL, of the B 3Π and A 3Φ states to deviate from 2.002 and 1.000. Nonadiabatic mixing with the nearby C 3Δ state is proposed as the cause of these deviations.
Original language | English (US) |
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Pages (from-to) | 567-573 |
Number of pages | 7 |
Journal | Astrophysical Journal |
Volume | 628 |
Issue number | 1 I |
DOIs | |
State | Published - Jul 20 2005 |
Keywords
- Astrochemistry
- Molecular data
- Molecular processes
- Stars: late-type
- Stars: magnetic fields
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science