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Astron. Astrophys. 322, L1-L4 (1997)
3. Analysis
The electronic ground state of NH is , so
that the rotational energy levels for exhibit a
fine structure leading to a triplet system in the observed spectrum.
For the lowest pure rotational transition, this fine structure triplet
is located at 946, 974, and 1000 GHz. Furthermore, the nonzero nuclear
spins of nitrogen and hydrogen give rise to magnetic dipole hyperfine
structure, which is further subdivided into Fermi contact
( ), dipole-dipole (t), and nuclear
spin-rotation ( ) interactions. In addition, the
14 N nucleus has nuclear spin and
hence causes an electric quadrupole interaction governed by the
parameter eQq. The Hamiltonian matrix elements needed to
determine the energy levels were calculated according to the coupling
scheme , , and
. Figure 2 shows the energy level diagram of the
transition.
![[FIGURE]](img28.gif) |
Fig. 2. Energy level diagram of the and 1 states of NH. The energy scale for the fine structure splitting is enlarged 10 times and the scale for the hyperfine structure is enlarged 2000 times with respect to the rotational energy levels. Transitions with relative intensities of 2% or more are indicated as listed in Table 1 (frequencies increase from left to right).
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We used the same computer program as previously employed by Saleck
et al. (1994a ) and Klaus et al. (1994, 1996 ), where the
explicit matrix elements can be found. The calculated spectral
frequencies were varied in the standard manner to determine the best
molecular constants. In the fitting procedure, the observed
frequencies were weighted proportionally to the inverse square of
their experimental uncertainties. For unresolved hyperfine splittings,
the frequencies were calculated as the weighted average of the
individual hyperfine components. The transitions already reported by
van den Heuvel et al. (1982 ) were replaced by our remeasured
frequencies, which were expected to be more reliable. The
observed-minus-calculated (O-C) values given in Table 1 show that
the experimental frequencies are reproduced very well within their
uncertainties, the value of the fit being 46
kHz.
In Table 2, the obtained constants are listed together with
their 1 uncertainties. In the analysis,
, the centrifugal distortion constant, was fixed
at 51.307 MHz. This value was derived from of
ND after measurement of its transition in the 1
THz region (to be published). A value for (N),
the spin-rotation constant involving the nitrogen nucleus, was
determined for the first time for NH by this study. The inclusion of
(H) yielded no significant improvement to the
fit.
![[TABLE]](img34.gif)
Table 2. Molecular constants for NH ( ) in its vibrational ground state
© European Southern Observatory (ESO) 1997
Online publication: June 5, 1998
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