Vladimír Spirko1, Takayoshi Amano, Wolfgang P Kraemer
1Institute for Astrophysics and Planetary Sciences, Ibaraki University, 2-1-1 Bunkyo, Mito 310-8512, Japan. spirko@marge.uochb.cas.cz
Calculations of spectral linewidths for the hydrogen cluster ion (H5+) and its deuterated isotopomer (D5+) suggest that observed spectral broadening is primarily due to spectral congestion, not predissociation.
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