Pure rotational as well as rovibrational data of several
isotopic species of ArH+ have been fit
simultaneously.
The J = 1 0 transition frequency was reported
in
(1) K. B. Laughlin, G. A. Blake, R. C. Cohen,
D. C. Hovde, and R. J. Saykally,
1987, Phys. Rev. Lett., 58, 996.
Additional lines up to J = 7 6 were
taken from
(2) J. M. Brown, D. A. Jennings, M. Vanek, L. R. Zink,
and K. Evenson,
1988, J. Mol. Spectrosc. 128, 587.
The J = 1 0 transition frequencies of three
ArD+ isotopic species involving 40Ar,
36Ar, and 38Ar, were published
by
(3) W. C. Bowman, G. M. Plummer, E. Herbst, and F. C. De Lucia,
1983, J. Chem. Phys. 79, 2093;
the reported uncertainties for the 40Ar and
36Ar species have been increased somewhat.
High-J pure rotational transition frequencies of
ArD+ were taken from
H. Odashima, A. Kozato, F. Matsushima, S. Tsunekawa,
and K. Takagi,
1999, J. Mol. Spectrosc. 195, 356.
High-J pure rotational transitions of ArH+
up to high vibrational states were detected in the lower
infrared region by
(5) D. J. Liu, W. C. Ho, and T. Oka,
1987, J. Chem. Phys. 87, 2442.
Rovibrational transitions of ArH+ were recorded
by
(6) J. W. Brault and S. P. Davis,
1982, Physica Scripta 25, 268.
Additional high-v transitions as well as transitions
of ArD+ were reported by
(7) J. W. C. Johns,
1984, J. Mol. Spectrosc. 106, 124.
Infrared data for 36ArH+ and
38ArH+ was provided by
(8) R. R. Filueira and C. E. Blom,
1988, J. Mol. Spectrosc. 127, 279.
There is great consistency among essentially all experimental
data. Therefore, it may well be that ion drift effects on the
reported frequencies are small. Nevertheless, all predictions
should be viewed with some caution, especially if the
calculated uncertainties exceed 2 MHz by far.
Experimental transitions frequencies with uncertainties larger
than 200 kHz have not been merged.
The dominant intersteller argon isotope is 36Ar.
The by far dominant isotope on Earth is 40Ar,
but it originates almost entirely from the radioactive decay
of 40K. Its relative abundance in the ISM is
almost negligible.
The partition function takes into account all vibrational states
used in the fit.
Non-zero contributions of individual vibrational states to the
partition function are given in parentheses.
The ab initio dipole moment was derived from the ArH+
ground state value of
(9) M. Cheng, J. M. Brown, P. Rosmus, R. Linguerri, N. Komiha,
and E. G. Myers,
2007, Phys. Rev. A 70, Art. No. 012502;
taking into account the D/H difference from
(10) P. Rosmus,
1979, Theor. Chim. Acta. 51, 359.
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