$^{g}$P. K. Carroll, P. McCormack and S.O. Connor, Astrophys. J. 208, 903 (1976) $^{h}$P. K. Carroll, and P. McCormack, Astrophys, J.(Letters) 177, L33 (1972). $^{i}$R. T. Carter and J. M Brown, J. Chem. Phys. 101(4), 2699 (1994) $^{j}$D. M. Goodridge, R. T. Carter, J. M. Brown and T. C. Steimle, (to be published in J. Chem. Phys. 106 (12), (1997).Author Institution: Department of Chemistry and Biochemistry, The Arizona State University; Department of Chemistry and Biochemistry, The Physical and Theoretical Chemistry LaboratoryThe visible spectrum of FeH is dominated by two strong band systems, one in the blue at around 493 nm and one in the green at around 532 nm $^{g,h}$. High resolution studies, earned out on room temperature samples, ha...
Author Institution: Department of Chemistry, University of Arizona; Department of Chemistry, Univers...
Author Institution: Department of Chemistry, The Johns Hopkin UniversityThe $^{6}\Pi - X^{6}\Delta$ ...
A high-resolution sunspot spectrum clearly shows the presence of the 9896 Å and 8691 Å bands of iron...
$^{a}$J. G. Phillips, S. P. Davis, B. Lindgren, and W. J. Balfour Astrophys. J. Supp. 65, 721 (1987)...
$^{1}$ J.G. Phillips, S.P. Davis, B. Lindgren and W.J. Balfour, Astrophys. J. Suppl., 65, 721 (1987)...
References D.M. Goodridge, D.F. Hullah and J.M. Brown, J. Chem. Phys., 108, 428-435 (1998). D.M. Goo...
Both FeH and FeH+ are predicted to be abundant in cool stellar atmospheres and proposed to be molecu...
$^{a}$ B. Pouilly, J. Schamps, D. J. W. Lumley and R. F. Barrow, J. Phys B: Atom. Molec. Phys., 11, ...
Iron monohydride, FeH, is an important astrophysical molecule observed in the cool outer layers of s...
Transitions between the spin-rotational levels of the FeH radical in the υ=0 level of the X4Δ ground...
The low-lying electronic states (X 4Δ, A 4Π, a 6Δ, b 6Π) of the iron monohydride radical, which are ...
This work targets laboratory studies of the Zeeman effects in selected transitions of the FeH radica...
FeOH is an iron-containing molecule that is a candidate for detection in interstellar space. It has ...
$^{1}$ P. McCormack and S. O'Connor. Ashon1 Astrphys. Suppl. 26.373 (1976).Author Institution: Physi...
Context. Lines of diatomic molecules are ideal tools for studying cool stellar atmospheres and the i...
Author Institution: Department of Chemistry, University of Arizona; Department of Chemistry, Univers...
Author Institution: Department of Chemistry, The Johns Hopkin UniversityThe $^{6}\Pi - X^{6}\Delta$ ...
A high-resolution sunspot spectrum clearly shows the presence of the 9896 Å and 8691 Å bands of iron...
$^{a}$J. G. Phillips, S. P. Davis, B. Lindgren, and W. J. Balfour Astrophys. J. Supp. 65, 721 (1987)...
$^{1}$ J.G. Phillips, S.P. Davis, B. Lindgren and W.J. Balfour, Astrophys. J. Suppl., 65, 721 (1987)...
References D.M. Goodridge, D.F. Hullah and J.M. Brown, J. Chem. Phys., 108, 428-435 (1998). D.M. Goo...
Both FeH and FeH+ are predicted to be abundant in cool stellar atmospheres and proposed to be molecu...
$^{a}$ B. Pouilly, J. Schamps, D. J. W. Lumley and R. F. Barrow, J. Phys B: Atom. Molec. Phys., 11, ...
Iron monohydride, FeH, is an important astrophysical molecule observed in the cool outer layers of s...
Transitions between the spin-rotational levels of the FeH radical in the υ=0 level of the X4Δ ground...
The low-lying electronic states (X 4Δ, A 4Π, a 6Δ, b 6Π) of the iron monohydride radical, which are ...
This work targets laboratory studies of the Zeeman effects in selected transitions of the FeH radica...
FeOH is an iron-containing molecule that is a candidate for detection in interstellar space. It has ...
$^{1}$ P. McCormack and S. O'Connor. Ashon1 Astrphys. Suppl. 26.373 (1976).Author Institution: Physi...
Context. Lines of diatomic molecules are ideal tools for studying cool stellar atmospheres and the i...
Author Institution: Department of Chemistry, University of Arizona; Department of Chemistry, Univers...
Author Institution: Department of Chemistry, The Johns Hopkin UniversityThe $^{6}\Pi - X^{6}\Delta$ ...
A high-resolution sunspot spectrum clearly shows the presence of the 9896 Å and 8691 Å bands of iron...