Deuterated methanol in the Orion compact ridge

被引:240
作者
Charnley, SB
Tielens, AGGM
Rodgers, SD
机构
[1] NASA,AMES RES CTR,DIV SPACE SCI,MOFFETT FIELD,CA 94035
[2] UNIV MANCHESTER,DEPT PHYS,MANCHESTER M60 1QD,LANCS,ENGLAND
关键词
ISM; abundances; clouds; molecules; molecular processes;
D O I
10.1086/310697
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have investigated the chemistry of hot cores containing methanol, formaldehyde, and their deuterated forms. We have computed the D fractionation ratios attainable by the addition of H and D atoms to CO on cold grain surfaces. We can easily reproduce the observed HDCO/H2CO and D2CO/H2CO ratios but find that, as there is an additional path to CH2DOH, the CH2DOH/CH3OD ratio is typically 3. This result is in conflict with the conclusion of Jacq et al. that the observed gas-phase CH2DOH/CH3OD ratio of approximate to 1.1-1.5 in the Orion Compact Ridge source is consistent with their production in grain mantles. We show that, when these mantles are evaporated, the CH2DOH/CH3OD ratio can be altered by gas-phase reactions that preferentially form CH3OD via reaction of H2DO+ with CH3OH. We find that an unrealistically high HDO/H2O ratio of approximate to 0.1 is necessary to drive the CH2DOH/CH3OD ratio to within the observed range. Before concluding that the observed gas-phase CH2DOH/CH3OD ratio is inconsistent with these grain-surface reactions, we recommend that more accurate determinations of this ratio be made in the Compact Ridge and in other hot cores.
引用
收藏
页码:L203 / L206
页数:4
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