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The Rotational Excitation Temperature of the 6614 DIB CarrierAnalysis of high spectral resolution observations of the lambda6614 DIB line profile show systematic variations in the positions of the peaks in the substructure of the profile. These variations can only be understood in the framework of rotational contours of large molecules, where the variations are caused by changes in the rotational excitation temperature. We show that the rotational excitation temperature for the DIB carrier is of the order 10-40 K - much lower than the gas kinetic temperature - indicating that for this particular DIB carrier angular momentum buildup is not very efficient. The rotational constant indicates that the carrier of this DIB is smaller than previously assumed:7-22 C atoms, depending on the geometry.
Document ID
20040084467
Acquisition Source
Ames Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Cami, J.
(NASA Ames Research Center Moffett Field, CA, United States)
Salama, F.
(NASA Ames Research Center Moffett Field, CA, United States)
Jimenez-Vicente, J.
(Granada Univ. Spain)
Galazutdinov, G.
(Korea Astronomy Observatory Daejon, Korea, Republic of)
Krelowski, J.
(Nicolaus Copernicus Univ. Torun, Poland)
Date Acquired
September 7, 2013
Publication Date
January 1, 2004
Subject Category
Fluid Mechanics And Thermodynamics
Funding Number(s)
PROJECT: RTOP 188-01-03-01
CONTRACT_GRANT: 2-P03D-019-23
Distribution Limits
Public
Copyright
Public Use Permitted.
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