Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 690, Issue 1, Pages L27-L30Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/690/1/L27
Keywords
astrochemistry; ISM: abundances; ISM: clouds; ISM: molecules; line: identification
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Funding
- Spanish Ministerio de Ciencia e Innovacion [AYA2003-2785, AYA2006-14876]
- ASTROCAM [S-0505/ESP-0237]
- Molecular Universe FP6 MCRTN
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We report on the first detection in space of fulminic acid, HCNO. This isomer of HNCO has been observed in three starless cores, B1, L1544, and L183, and in the low-mass star-forming region L1527 with a measured abundance ratio of HNCO/HCNO between 40 and 70. However, HCNO was not detected toward the direction of the cyanopolyyne peak of TMC-1 or toward the Orion Hot Core region. The derived HNCO/HCNO abundance ratio in these cases is greater than 350 and 1000 in TMC-1 and Orion, respectively. We find that CH2 + NO -> HCNO + H is a key reaction for the formation of fulminic acid. A value of 5.5 x 10(-12) cm(3) s(-1) of the corresponding reaction rate coefficient, as given by Miller et al., allows us to reproduce the observed abundances of fulminic acid in both the observed dark clouds and low-mass star-forming core, where the determined abundance of HNCO in these regions with respect to molecular hydrogen is 1-5 x 10(-10).
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