المساق
arXiv 2015-01-06 DOI 10.1088/0067-0049/216/2/30 0 مشاهدة

Vibrationally Excited C₄H

Cooksy, Andrew L. · Gottlieb, C. A. · Killian, T. C. · Thaddeus, P. · Patel, Nimesh A. · Young, Ken H. · McCarthy, M. C.

الأصل · EN

Rotational spectra in four new excited vibrational levels of the linear carbon chain radical C₄H radical were observed in the millimeter band between 69 and 364 GHz in a low pressure glow discharge, and two of these were observed in a supersonic molecular beam between 19 and 38 GHz. All have rotational constants within 0.4% of the ²Σ+ ground vibrational state of C₄H and were assigned to new bending vibrational levels, two each with ²Σ and ²Π vibrational symmetry. The new levels are tentatively assigned to the 1ν₆ and 1ν₅ bending vibrational modes (both with ²Π symmetry), and the 1ν₆ + 1ν₇ and 1ν₅ + 1ν₆ combination levels (²Σ symmetry) on the basis of the derived spectroscopic constants, relative intensities in our discharge source, and published laser spectroscopic and quantum calculations. Prior spectroscopic constants in the 1ν₇ and 2ν₇ levels were refined. Also presented are interferometric maps of the ground state and the 1ν₇ level obtained with the SMA near 257 GHz which show that C₄H is present near the central star in IRC+10216. We found no evidence with the SMA for the new vibrationally excited levels of C₄H at a peak flux density averaged over a 3′′ synthesized beam of ≥ 0.15 Jy/beam in the 294-296 and 304-306 GHz range, but it is anticipated that rotational lines in the new levels might be observed in IRC+10216 when ALMA attains its full design capability.

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