1992•Indian Institute of AstrophysicsRequires access
Can HeH(+) molecule be present in solar photosphere
V. P. Gaur, G. C. Joshi, M. C. Pande
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Abstract
The equivalent widths of the P and R branch lines of the fundamental vibration-rotation band arising from the ground state of HeH(+) have been calculated in a chosen photospheric model. The resulting equivalent widths suggest that the solar spectrum in the infrared region should be searched for, resolving the question regarding the presence or absence of HeH(+) in the sun