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24 April 2024 |
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Article overview
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Discovery of Interstellar Propylene (CH_2CHCH_3): Missing Links in
Interstellar Gas-Phase Chemistry | | N. Marcelino
; J. Cernicharo
; M. Agundez
; E. Roueff
; M. Gerin
; J. Martin-Pintado
; R. Mauersberger
; C. Thum
; | | Date: |
9 Jul 2007 | | Abstract: | We report the discovery of propylene (also called propene, CH_2CHCH_3) with
the IRAM 30-m radio telescope toward the dark cloud TMC-1. Propylene is the
most saturated hydrocarbon ever detected in space through radio astronomical
techniques. In spite of its weak dipole moment, 6 doublets (A and E species)
plus another line from the A species have been observed with main beam
temperatures above 20 mK. The derived total column density of propylene is 4
10^13 cm^-2, which corresponds to an abundance relative to H_2 of 4 10^-9,
i.e., comparable to that of other well known and abundant hydrocarbons in this
cloud, such as c-C_3H_2. Although this isomer of C_3H_6 could play an important
role in interstellar chemistry, it has been ignored by previous chemical models
of dark clouds as there seems to be no obvious formation pathway in gas phase.
The discovery of this species in a dark cloud indicates that a thorough
analysis of the completeness of gas phase chemistry has to be done. | | Source: | arXiv, arxiv.0707.1308 | | Services: | Forum | Review | PDF | Favorites | |
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