Gauche ethyl alcohol: Laboratory assignments and interstellar identification

被引:66
作者
Pearson, JC
Sastry, KVLN
Herbst, E
DeLucia, FC
机构
[1] UNIV NEW BRUNSWICK,DEPT PHYS,FREDERICTON,NB E3B 5A3,CANADA
[2] OHIO STATE UNIV,DEPT PHYS,COLUMBUS,OH 43210
[3] OHIO STATE UNIV,DEPT ASTRON,COLUMBUS,OH 43210
关键词
ISM; molecules; line; identification; molecular data; molecular processes radio lines;
D O I
10.1086/303967
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Ethyl alcohol (ethanol) is known to possess a pair of closely spaced excited torsional substates (gauche+, gauche-) at an energy of approximately 57 K above the ground (trans) torsional substate. We report an extended analysis of some gauche- -gauche+ Q-branch (Delta J = 0) transitions with a three-substate fixed frame axis method (FFAM) Hamiltonian. Our approach accounts for complex trans-gauche interactions for the first time. In addition, we are able to obtain intensities for perturbed rotational transitions, and to determine the trans to gauche+ separation to be 1185399.1 MHz. A complete ground state rotational-torsional partition function accounting for the previously neglected gauche substates is presented. Based on our analysis, a total of 14 U lines obtained towards Orion KL can now be assigned to gauche substates of ethanol. Analysis of these lines yields a rotational temperature of 223 K and a total (trans + gauche) column density of 7.0 x 10(15) cm(-2). The column density is in reasonable agreement with the recent value of 2-3 x 10(15) cm(-2) based on observations of trans-ethanol by Ohishi et al., although there is some disparity in the rotational temperatures, Eight additional fi lines in the literature are assigned to transitions of gauche ethanol.
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页码:420 / 431
页数:12
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