Rotational excitation of formaldehyde by hydrogen molecules: ortho-H_2CO at low temperature
暂无分享,去创建一个
[1] J. Noga,et al. R12-calibrated H2O-H2 interaction: full dimensional and vibrationally averaged potential energy surfaces. , 2008, The Journal of chemical physics.
[2] K. Menten,et al. Formaldehyde Densitometry of Starburst Galaxies , 2007, 0710.2115.
[3] M. Dubernet,et al. Quasi-classical rate coefficient calculations for the rotational (de)excitation of H2O by H2 , 2007, 0708.0345.
[4] N. Feautrier,et al. Rotationally inelastic collisions of SO(X3Sigma-) with H2: potential energy surface and rate coefficients for excitation by para-H2 at low temperature. , 2007, The Journal of chemical physics.
[5] J. Noga,et al. Influence of a new potential energy surface on the rotational (de)excitation of H2O by H2 at low temperature , 2006 .
[6] L. Wiesenfeld,et al. Rotational excitation of HC3N by H2 and He at low temperatures , 2006, physics/0611258.
[7] J. Noga,et al. On the role of high excitations in the intermolecular potential of H2–CO , 2006 .
[8] J. Pety,et al. Comparative chemistry of diffuse clouds V. Ammonia and formaldehyde , 2006 .
[9] P. Jankowski,et al. Improved low-temperature rate constants for rotational excitation of CO by H 2 , 2006, astro-ph/0601384.
[10] K. L. Baluja,et al. Electron-impact study of formaldehyde using the R-matrix method , 2005 .
[11] P. Jankowski,et al. A new ab initio interaction energy surface and high-resolution spectra of the H2-CO van der Waals complex. , 2005, The Journal of chemical physics.
[12] J. Tennyson,et al. A full nine-dimensional potential-energy surface for hydrogen molecule-water collisions. , 2005, The Journal of chemical physics.
[13] N. Biver,et al. Origin of the formaldehyde (H2CO) extended source in comet C/1995 O1 (Hale-Bopp) , 2004 .
[14] L. Wiesenfeld,et al. Ambiguities in the semiclassical assignment of the asymmetric rotor rotational quantum numbers. , 2004, The Journal of chemical physics.
[15] E. Caux,et al. Theoretical H2CO emission from protostellar envelopes , 2003, astro-ph/0506144.
[16] A. Tielens,et al. The H2CO abundance in the inner warm regions of low mass protostellar envelopes , 2003, astro-ph/0310536.
[17] D. Teyssier,et al. The Hot Core around the Low-Mass Protostar IRAS 16293–2422: Scoundrels Rule! , 2003 .
[18] Martyn D. Wheeler,et al. A new potential energy surface for He–H2CO , 2003 .
[19] L. Loinard,et al. CO Depletion and Deuterium Fractionation in Prestellar Cores , 2003, astro-ph/0301651.
[20] M. Dubernet,et al. Collisional excitation rates of H2O with H2. I. Pure rotational excitation rates with para-H2 at very low temperature , 2002 .
[21] H. Liszt,et al. Comparative chemistry of diffuse clouds. IV: CH , 2002, astro-ph/0206119.
[22] A. Tielens,et al. Extended D2CO emission: The smoking gun of grain surface-chemistry , 2001 .
[23] F. D. De Lucia,et al. Helium and Hydrogen Induced Rotational Relaxation of H2CO Observed at Temperatures of the Interstellar Medium , 2000 .
[24] S. Green,et al. Collisional Excitation of H 2O by H 2 Molecules , 1996 .
[25] Gisbert Winnewisser,et al. The Ground State Rotational Spectrum of Formaldehyde , 1996 .
[26] K. Szalewicz,et al. On the effectiveness of monomer‐, dimer‐, and bond‐centered basis functions in calculations of intermolecular interaction energies , 1995 .
[27] G. Blake,et al. Molecular Abundances and Low-Mass Star Formation. II. Organic and Deuterated Species toward IRAS 16293-2422 , 1995 .
[28] J. Noga,et al. Coupled cluster theory that takes care of the correlation cusp by inclusion of linear terms in the interelectronic coordinates , 1994 .
[29] A. D. McLean,et al. Anisotropic rigid rotor potential energy function for H2O–H2 , 1994 .
[30] J. Mangum,et al. Formaldehyde as a probe of physical conditions in dense molecular clouds , 1993 .
[31] S. Green. Collisional excitation of formaldehyde in 'hot' interstellar molecular regions , 1991 .
[32] D. Clouthier,et al. The Spectroscopy of Formaldehyde and Thioformaldehyde , 1983 .
[33] J. Krolik,et al. Hydrogen emission-line spectra in quasars and active galactic nuclei , 1978 .
[34] W. A. Lester,et al. Collisional excitation of interstellar formaldehyde , 1978 .
[35] W. Lester,et al. Coupled‐channel study of rotational excitation of a rigid asymmetric top by atom impact: (H2CO,He) at interstellar temperatures , 1976 .
[36] W. Lester,et al. Effect of electron correlation on the H2CO‐He interaction potential , 1975 .
[37] W. Miller,et al. Cooling of the 6-centimeter and 2-centimeter doublets of interstellar H$sub 2$CO by collision: an accurate quantum-mechanical calculation , 1975 .
[38] D. Lester,et al. Search for polarimetric variations in the close binary GK Cephei , 1975 .
[39] J. L. Duncan,et al. The ground-state average and equilibrium structures of formaldehyde and ethylene , 1974 .
[40] W. Miller,et al. Semiclassical treatment of atom‐asymmetric rotor collisions; rotational excitation of formaldehyde at low energies , 1974 .
[41] C. Townes,et al. A pumping mechanism for anomalous microwave absorption in formaldehyde in interstellar space. , 1969 .
[42] J. Tennyson,et al. Electron-impact rotational excitation of water , 2004 .
[43] D. Buhl,et al. MICROWAVE DETECTION OF INTERSTELLAR FORMALDEHYDE. , 1969 .