On the detectibility of HeH(+) in the solar photospheric spectrum

Details On the detectibility of HeH(+) in the solar photospheric spectrum On the detectibility of HeH(+) in the solar photospheric spectrum

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994basi...22..143s&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 22, no. 2, p. 143-147

Astronomy and Astrophysics

Astronomy

Helium Compounds, Hydrogen Ions, Photosphere, Solar Spectra, Astronomical Catalogs, Rotational Spectra, Spaceborne Astronomy, Vibrational Spectra

Scientific paper

In a recent publication of the Bulletin of the Astronomical Society of India, the possibility of detection of the (1-0) vibration-rotation lines of HeH(+) molecules in the solar photospheric spectrum has been suggested. Taking cue, the Photometric Atlas of the solar Spectrum from 1850 to 10,000 1 cm was scanned for the suggested lines in the present preliminary ivestigation. It is tentatively concluded that (1) it seems rather difficult to detect the HeH(+) lines and (2) observations from above the terrestrial atmosphere may be required for firm conclusions.

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