[1] Calculated High Temperature Partition Function and Related
Thermodynamic Data for H216O
Harris, G. J., Viti, S., Mussa, H. Y., & Tennyson, J.
(1998) J.
Chem. Phys. 109, 7197.
Online
OR PDF (117 kb).
[2] Ab Initio Global Potential, Dipole Adiabatic, and
Relativistic
Correction Surfaces for the HCN-HNC System
Van Mourik, T., Harris, G. J., Polyansky, O. L., Tennyson, J.,
Csa'sza'r, A. G., & Knowles, P. J.
(2001) J.
Chem. Phys. 115, 3706.
Online
OR PDF (132 kb). Online
data.
[3] Ab Initio Rotation-Vibration Spectra of HCN and HNC
Harris, G. J., Polyansky, O. L., and Tennyson, J.
(2002) Spectrochimica
Acta Part A. 58, 673.
Online
OR PDF (272 kb).
[4] An Ab Initio HCN/HNC Rotational-Vibrational Line List and
Opacity
Function for Astronomy.
Harris, G. J.
(2002) Ph.D. Thesis. University of London. PDF
(5.9 Mb)
[5] Opacity Data for HCN and HNC from a New Ab Initio Linelist
Harris, G. J., Polyansky, O. L., & Tennyson, J.
(2002) Astrophysical
Journal, 578, 657.
Online
OR PDF (261 kb). Online data
[6] Temperature Dependent Partition Function and Equilibrium
Constant
for HCN and HNC.
Barber, R. J., Harris, G. J., & Tennyson, J.
(2002) J.
Chem. Phys. 117, 11239.
Online
OR PDF (117 kb).
[7] The Identification of HCN and HNC in Carbon Stars: Model
Atmospheres, Synthetic Spectra and Fits to observation in the 2.7 to
4.0 micron Region.
Harris, G. J., Pavlenko, Ya. V., Jones, H. R. A., & Tennyson, J.
(2003) MNRAS
344, 1107.
Online
OR PDF (312 kb).
[8] The effect of the electron donor H3+ on
the
pre-main and Main Sequence evolution of low mass zero metallicity stars.
Harris, G. J., Lynas-Gray, A. E., Miller, S., & Tennyson, J.
(2004) Astrophysical
Journal, 600, 1025.
Online
OR PDF (333 kb). Online
data.
[9] DVR3D: A Program Suite for the Calculation of
Rotation-vibration
Spectra of Triatomic Molecules.
Tennyson, J., Kostin, M. A., Barletta, P., Harris, G. J., Ramanlal,
J., Polyansky, O. L., & Zobov, N. F.
(2004) Computer
Physics Communications, 163, 85.
Online
OR PDF (367 kb).
[10] The role of HeH+ in cool helium rich white dwarfs.
Harris, G. J., Lynas-Gray, A. E., Miller, S., & Tennyson,
J.
(2004) Astrophysical
Journal, 617, L143.
Online
OR PDF (106 kb).
[11] Calculated spectra for HeH+ and its effect on the
opacity of cool metal poor stars.
Engel, E. A., Doss, N., Harris, G. J., Tennyson, J..
(2005) MNRAS, 357, 471.
Online,
OR PDF (317 kb). Online
data
[12] Status of the physics of
substellar objects.
Jones, H. R. A., Viti, S., Tennyson,
J., Barber, R. J., Harris, G. J., et al.
(2005) Astronomische Nachrichten, 326, 920.
Online,
OR PDF (240 kb).
[13] Improved HCN/HNC linelist,
model
atmospheres and synthetic spectra for WZ Cas.
Harris, G. J., Tennyson, J.,
Kaminsky, B. M., Pavlenko, Ya. V., Jones, H. R. A.
(2006) MNRAS, 367, 400.
Online,
OR PDF (725 kb). Online
data
[14] A high-accuracy computed water
line
list.
Barber, R. J., Tennyson, J., Harris,
G. J., Tolchenov, R. N..
(2006) MNRAS, 368, 1087.
Online,
OR PDF (180 kb). Online data
[15] Non-grey hydrogen burning
evolution
of sub-Solar mass Population III stars.
Harris, G. J., Lynas-Gray, A.E.,
Miller, S., & Tennyson, J.
(2007) MNRAS, 374, 337.
Online,
OR PDF (246 kb).