J/ApJ/813/96             CO ro-vibrational transitions             (Song+, 2015)

Quantum calculation of inelastic CO collisions with H. III. Rate coefficients for ro-vibrational transitions. Song L., Balakrishnan N., WalkerK.M., Stancil P.C., Thi W.F.,Kamp I., van der Avoird A., Groenenboom G.C. <Astrophys. J., 813, 96 (2015)> =2015ApJ...813...96S 2015ApJ...813...96S (SIMBAD/NED BibCode)
ADC_Keywords: Atomic physics Keywords: astronomical databases: miscellaneous; ISM: molecules; molecular data; molecular processes; photon-dominated region, PDR; protoplanetary disks Abstract: We present calculated rate coefficients for ro-vibrational transitions of CO in collisions with H atoms for a gas temperature range of 10K≤T≤3000K, based on the recent three-dimensional ab initio H-CO interaction potential of Song et al. (2013JPCA..117.7571S 2013JPCA..117.7571S). Rate coefficients for ro-vibrational v=1,j=0-30->v'=0,j' transitions were obtained from scattering cross sections previously computed with the close-coupling (CC) method by Song et al. (2015JChPh.142t4303S 2015JChPh.142t4303S). Combining these with the rate coefficients for vibrational v=1-5->v'<v quenching obtained with the infinite-order sudden approximation, we propose a new extrapolation scheme that yields the rate coefficients for ro-vibrational v=2-5,j=0-30->v',j' de-excitation. Cross sections and rate coefficients for ro-vibrational v=2,j=0-30->v'=1,j' transitions calculated with the CC method confirm the effectiveness of this extrapolation scheme. Our calculated and extrapolated rates are very different from those that have been adopted in the modeling of many astrophysical environments. The current work provides the most comprehensive and accurate set of ro-vibrational de-excitation rate coefficients for the astrophysical modeling of the H-CO collision system. The application of the previously available and new data sets in astrophysical slab models shows that the line fluxes typically change by 20%-70% in high temperature environments (800K) with an H/H2 ratio of 1; larger changes occur for lower temperatures. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 195 1096 Rate coefficients from close-coupling (CC) calculations for ro-vibrational transitions from v=1,j=0-30 to v'=0,j' in the temperature range T=10-3000K table2.dat 195 1096 Rate coefficients from close-coupling (CC) calculations for ro-vibrational transitions from v=2,j=0-30 to v'=1,j' in the temperature range T=10-3000K -------------------------------------------------------------------------------- See also: J/A+A/492/257 : Collisional excitation of water in warm media (Faure+, 2008) J/A+A/432/369 : Leiden Atomic and Molecular Database (LAMDA) (Schoeier+, 2005) J/A+AS/117/561 : Rovibrational dipole matrix elements for CO (Hure+ 1996) J/A+AS/117/557 : Einstein coefficients for CO transitions (Chandra+ 1996) J/ApJS/95/535 : Infrared CO line list for X 1Σ+ state (Goorvitch, 1994) Byte-by-byte Description of file: table[12].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- j1lev [0/30] rotational level in vibration level (v=1 for table1 or v=2 for table2) 4- 5 I2 --- j0lev [0/42] rotational level in vibration level (v=0 for table1 or v=1 for table2) 7- 15 E9.3 cm3/s rdrc10k ro-vibrational de-excitation rate coeff at 10K 17- 25 E9.3 cm3/s rdrc20k ro-vibrational de-excitation rate coeff at 20K 27- 35 E9.3 cm3/s rdrc30k ro-vibrational de-excitation rate coeff at 30K 37- 45 E9.3 cm3/s rdrc40k ro-vibrational de-excitation rate coeff at 40K 47- 55 E9.3 cm3/s rdrc50k ro-vibrational de-excitation rate coeff at 50K 57- 65 E9.3 cm3/s rdrc60k ro-vibrational de-excitation rate coeff at 60K 67- 75 E9.3 cm3/s rdrc70k ro-vibrational de-excitation rate coeff at 70K 77- 85 E9.3 cm3/s rdrc80k ro-vibrational de-excitation rate coeff at 80K 87- 95 E9.3 cm3/s rdrc90k ro-vibrational de-excitation rate coeff at 90K 97-105 E9.3 cm3/s rdrc100k ro-vibrational de-excitation rate coeff at 100K 107-115 E9.3 cm3/s rdrc200k ro-vibrational de-excitation rate coeff at 200K 117-125 E9.3 cm3/s rdrc300k ro-vibrational de-excitation rate coeff at 300K 127-135 E9.3 cm3/s rdrc500k ro-vibrational de-excitation rate coeff at 500K 137-145 E9.3 cm3/s rdrc700k ro-vibrational de-excitation rate coeff at 700K 147-155 E9.3 cm3/s rdrc1000k ro-vibrational de-excitation rate coeff at 1000K 157-165 E9.3 cm3/s rdrc1500k ro-vibrational de-excitation rate coeff at 1500K 167-175 E9.3 cm3/s rdrc2000k ro-vibrational de-excitation rate coeff at 2000K 177-185 E9.3 cm3/s rdrc2500k ro-vibrational de-excitation rate coeff at 2500K 187-195 E9.3 cm3/s rdrc3000k ro-vibrational de-excitation rate coeff at 3000K -------------------------------------------------------------------------------- History: From electronic version of the journal References: Yang et al. Paper I. 2013ApJ...771...49Y 2013ApJ...771...49Y Walker et al. Paper II. 2015ApJ...811...27W 2015ApJ...811...27W
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 15-Feb-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line