Asymptotic Expansion of the Partition Function of the Asymmetric Top

1951 ◽  
Vol 19 (9) ◽  
pp. 1131-1133 ◽  
Author(s):  
Kenneth F. Stripp ◽  
John G. Kirkwood
1991 ◽  
Vol 95 (11) ◽  
pp. 8374-8389 ◽  
Author(s):  
J. M. L. Martin ◽  
J. P. François ◽  
R. Gijbels

2019 ◽  
Vol 627 ◽  
pp. A65 ◽  
Author(s):  
M. Carvajal ◽  
C. Favre ◽  
I. Kleiner ◽  
C. Ceccarelli ◽  
E. A. Bergin ◽  
...  

We emphasize that the completeness of the partition function, that is, the use of a converged partition function at the typical temperature range of the survey, is very important to decrease the uncertainty on this quantity and thus to derive reliable interstellar molecular densities. In that context, we show how the use of different approximations for the rovibrational partition function together with some interpolation and/or extrapolation procedures may affect the estimate of the interstellar molecular column density. For that purpose, we apply the partition function calculations to astronomical observations performed with the IRAM-30 m telescope towards the NGC 7538–IRS1 source of two N-bearing molecules: isocyanic acid (HNCO, a quasilinear molecule) and methyl cyanide (CH3CN, a symmetric top molecule). The case of methyl formate (HCOOCH3), which is an asymmetric top O-bearing molecule containing an internal rotor is also discussed. Our analysis shows that the use of different partition function approximations leads to relative differences in the resulting column densities in the range 9–43%. Thus, we expect this work to be relevant for surveys of sources with temperatures higher than 300 K and to observations in the infrared.


1933 ◽  
Vol 29 (3) ◽  
pp. 407-407 ◽  
Author(s):  
Irene E. Viney

I am indebted to Mr L. Kassel of the Department of Commerce, U.S.A., for pointing out an error of computation in a recent paper in these Proceedings.The asymptotic expansion for the partition function should readwhere


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