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Detection of interstellar methyldiacetylene (CH/sub 3/C/sub 4/H)

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/184312· OSTI ID:6176050
A new interstellar molecule methyldiacetylene (CH/sub 3/C/sub 4/H) has been detected in the molecular cloud TMC-1. The J = 6..-->..5 and J = 5..-->..4 transitions have been observed in their K = 0 and K = 1 components. An assumed value of radial velocity V/sub LSR/ = +5.8 +- 0.2 km s/sup -1/ for TMC-1 yields molecular rotational constants B/sub 0/ = 2035.746 +- 0.005 MHz, D/sub J/ = 0.06 +- 0.09 kHz, and D/sub J//sub K/ = 19.8 +- 0.3 kHz, in good agreement with laboratory values. The total column density of CH/sub 3/C/sub 4/H lies in the range 2.0 x 10/sup 13/ cm/sup -2/< or =(CH/sub 3/C/sub 4/H)< or = 3 x 10/sup 13/ cm/sup -2/ for rotational temperatures from 4 K to 6 K. By comparison with CH/sub 3/C/sub 2/H, we conclude that the chemical process whereby two carbon atoms are added to the chain to make CH/sub 3/C/sub 4/H results in a decrease in abundance by a factor of 2-4, similar to the situation for linear cyanopolyynes. Because this relative abundance factor of approximately 3 is common to several different types of carbon chain molecules, we suggest that it reflects the relative abundance of pure carbon chains of different lengths. We also infer that the relative abundances (HC/sub 2/H)/(H/sub 2/) and (HC/sub 4/H)/(H/sub 2/) are 0.5 x 10/sup -6/ and 0.2 x 10/sup -6/, respectively, for TMC-1.
Research Organization:
Herzberg Institute of Astrophysics, National Research Council of Canada, Ottawa
OSTI ID:
6176050
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 282:2; ISSN AJLEA
Country of Publication:
United States
Language:
English